24 results
49 Case Study: Cognitive Deficits Associated with Norrie Disease
- Amy LeRoy, Khushnoo K Indorewalla, Richard Phenis, Joyce Yi Hsuan Ku
-
- Journal:
- Journal of the International Neuropsychological Society / Volume 29 / Issue s1 / November 2023
- Published online by Cambridge University Press:
- 21 December 2023, pp. 655-656
-
- Article
-
- You have access Access
- Export citation
-
Objective:
Norrie disease is a rare, x-linked recessive genetic disorder associated with an NDP gene mutation. Males are predominantly affected. Typical symptoms include vision loss around the time of birth and progressive hearing loss. Cognitive and behavioral abnormalities also occur in 30-50% of individuals, including developmental delays, intellectual disability, cognitive regression, psychosis, and aggression. There is limited research, however, examining the neuropsychological deficits in adulthood resulting from Norrie disease, especially with neuropsychological data and in individuals without other neurological manifestations of the disease, such as seizures. Here, we present the neurocognitive profile of a patient with Norrie disease who presented for a cognitive evaluation in adulthood due to report of more recent memory decline.
Participants and Methods:Mr. Smith is a Caucasian male in his mid-40's who previously underwent genetic testing and was subsequently diagnosed with Norrie disease. As a result of his diagnosis, he experienced complete vision loss since birth and bilateral hearing loss that began in childhood and gradually worsened in adolescence. Medical history was otherwise unremarkable. Developmental milestones were met on time. Historical intelligence testing conducted in elementary school revealed borderline on one intelligence test to high average performance on other intelligence tests. However, he was retained grades several times due to factors such as behavioral disruptions and academic difficulties. He had been employed as an assembly line worker for many years, but had not worked for 10 years prior to the neuropsychological evaluation. Emotionally, he had a longstanding history of anxiety and endorsed mild anxiety and depression at the time of the evaluation. The patient first noticed memory difficulties in adolescence then noticed further decline four years prior to the neuropsychological evaluation (around when he received a left-ear cochlear implant), which had remained stable since onset.
Results:In the context of low average premorbid intellectual functioning, Mr. Smith's neurocognitive profile was notable for difficulties with alphanumeric set-shifting and abstract thinking, with otherwise preserved cognitive functioning. Weaknesses observed on testing may have represented longstanding weaknesses and did not rise to the level of a cognitive disorder. Affective distress was also suspected to have accounted for some of the cognitive lapses the patient reported experiencing with day-to-day functioning.
Conclusions:The current poster aims to contribute to the limited body of literature examining neuropsychological deficits in adulthood resulting from Norrie disease. This is especially critical given that the long-term cognitive dysfunction of this disorder is relatively unknown and could negatively impact patients' quality of life over time.
P.070 Introducing Stroke Endovascular Thrombectomy Into A Smaller Canadian Site, Is It Safe?
- K Attwell-Pope, A Penn, A Henri-Bhargava, S Greek, M Penn, J LeRoy, M Bibok
-
- Journal:
- Canadian Journal of Neurological Sciences / Volume 48 / Issue s3 / November 2021
- Published online by Cambridge University Press:
- 05 January 2022, p. S39
-
- Article
-
- You have access Access
- Export citation
-
Background: Success of Endovascular Thrombectomy (EVT) requires ultra-fast access to specialized neuro imaging, neurological assessment and an angio suite with interventional radiologists. Prior access was via transport to Vancouver and outcomes were poor, with a high rate of disability or death. This appeared primarily due to long delays. Methods: Quality control process, in parallel to the introduction of a new intervention, EVT, to Vancouver Island, to determine if this intervention could be delivered with reasonable safety and good outcomes. Patients receiving EVT from May, 2016 until Sep, 2019 are included, with 90-day outcomes. Data was collected by stroke nurses. Results: The proportion of patients having a good outcome was comparable to that of the major clinical trial involving Canadian academic centres. The proportion sustaining a poor outcome was comparable to the control group in that trial population (who still received tPA treatment where possible). This was despite a median age 4.5 years greater than in that trial. Conclusions: EVT required coordination of multiple services. Victoria General Hospital performance in terms of speed to treatment was slower than in the published trials. This is a factor in determining outcome and is therefore an important quality improvement target moving forward.
Variation of the molecular cloud lifecycle across the nearby galaxy population
- Jaeyeon Kim, Mélanie Chevance, J. M. Diederik Kruijssen, Adam K. Leroy
-
- Journal:
- Proceedings of the International Astronomical Union / Volume 17 / Issue S373 / August 2021
- Published online by Cambridge University Press:
- 09 June 2023, pp. 299-305
- Print publication:
- August 2021
-
- Article
-
- You have access Access
- Open access
- Export citation
-
The processes of star formation and feedback take place on the scales of giant molecular clouds (GMCs; ~ 100 pc) within galaxies and play a major role in governing galaxy evolution. By applying a robust statistical method to PHANGS observations, we systematically measure the evolutionary timeline from molecular clouds to exposed young stellar regions, across an unprecedented sample of 54 galaxies. These timescales depend on galaxy environment, revealing the role of galactic-scale dynamical processes in the small-scale GMC evolution. Furthermore, in the 5 nearest galaxies of our sample, we have refined the GMC timeline further and established the duration of the heavily obscured phase, using 24 μm emission. These results represent a major first step towards a comprehensive picture of cloud assembly and feedback, which will be extended to 19 more galaxies with our ongoing JWST Large Program.
Death anxiety in patients with primary brain tumor: Measurement, prevalence, and determinants
- Ashlee R. Loughan, Mariya Husain, Scott G. Ravyts, Kelcie D. Willis, Sarah Ellen Braun, Julia K. Brechbiel, Farah J. Aslanzadeh, Gary Rodin, Dace S. Svikis, Leroy Thacker
-
- Journal:
- Palliative & Supportive Care / Volume 19 / Issue 6 / December 2021
- Published online by Cambridge University Press:
- 22 June 2021, pp. 672-680
-
- Article
- Export citation
-
Objective
This study investigated death anxiety in patients with primary brain tumor (PBT). We examined the psychometric properties of two validated death anxiety measures and determined the prevalence and possible determinants of death anxiety in this often-overlooked population.
MethodsTwo cross-sectional studies in neuro-oncology were conducted. In Study 1, 81 patients with PBT completed psychological questionnaires, including the Templer Death Anxiety Scale (DAS). In Study 2, 109 patients with PBT completed similar questionnaires, including the Death and Dying Distress Scale (DADDS). Medical and disease-specific variables were collected across participants in both studies. Psychometric properties, including construct validity, internal consistency, and concurrent validity, were investigated. Levels of distress were analyzed using frequencies, and determinants of death anxiety were identified using logistic regression.
ResultsThe DADDS was more psychometrically sound than the DAS in patients with PBT. Overall, 66% of PBT patients endorsed at least one symptom of distress about death and dying, with 48% experiencing moderate-severe death anxiety. Generalized anxiety symptoms and the fear of recurrence significantly predicted death anxiety.
Significance of resultsThe DADDS is a more appropriate instrument than the DAS to assess death anxiety in neuro-oncology. The proportion of patients with PBT who experience death anxiety appears to be higher than in other advanced cancer populations. Death anxiety is a highly distressing symptom, especially when coupled with generalized anxiety and fears of disease progression, which appears to be the case in patients with PBT. Our findings call for routine monitoring and the treatment of death anxiety in neuro-oncology.
Codium-like taxa from the Silurian of North America: morphology, taxonomy, paleoecology, and phylogenetic affinity
- Steven T. LoDuca, Anthony L. Swinehart, Matthew A. LeRoy, Denis K. Tetreault, Shawn Steckenfinger
-
- Journal:
- Journal of Paleontology / Volume 95 / Issue 2 / March 2021
- Published online by Cambridge University Press:
- 29 October 2020, pp. 207-235
-
- Article
- Export citation
-
A 1901 report by the Smithsonian Custodian of Paleozoic Plants noted that the nonbiomineralized taxa Buthotrephis divaricata White, 1901, B. newlini White, 1901, and B. lesquereuxi Grote and Pitt, 1876, from the upper Silurian of the Great Lakes area, shared key characteristics in common with the extant green macroalga Codium. A detailed reexamination of these Codium-like taxa and similar forms from the lower Silurian of Ontario, New York, and Michigan, including newly collected material of Thalassocystis striata Taggart and Parker, 1976, aided by scanning electron microscopy and stable carbon isotope analysis, provides new data in support of an algal affinity. Crucially, as with Codium, the originally cylindrical axes of all of these taxa consist of a complex internal array of tubes divided into distinct medullary and cortical regions, the medullary tubes being arranged in a manner similar to those of living Pseudocodium. In view of these findings, the three study taxa originally assigned to Buthotrephis, together with Chondrites verus Ruedemann, 1925, are transferred to the new algal taxon Inocladus new genus, thereby establishing Inocladus lesquereuxi new combination, Inocladus newlini new comb., Inocladus divaricata new comb., and Inocladus verus new comb. Morphological and paleoecological data point to a phylogenetic affinity for Inocladus n. gen. and Thalassocystis within the Codium-bearing green algal order Bryopsidales, but perhaps nested within an extinct lineage. Collectively, this material fits within a large-scale pattern of major macroalgal morphological diversification initiated in concert with the Great Ordovician Biodiversification Event and apparently driven by a marked escalation in grazing pressure.
UUID: http://zoobank.org/97c5c737-b291-41a2-aceb-f398cac9537a
How do we improve adolescent diet and physical activity in India and sub-Saharan Africa? Findings from the Transforming Adolescent Lives through Nutrition (TALENT) consortium
- ME Barker, P Hardy-Johnson, S Weller, A Haileamalak, L Jarju, J Jesson, GV Krishnaveni, K Kumaran, V Leroy, SE Moore, SA Norris, S Patil, SA Sahariah, K Ward, CS Yajnik, CHD Fall
-
- Journal:
- Public Health Nutrition / Volume 24 / Issue 16 / November 2021
- Published online by Cambridge University Press:
- 28 October 2020, pp. 5309-5317
-
- Article
-
- You have access Access
- HTML
- Export citation
-
Objective:
Adolescent diet, physical activity and nutritional status are generally known to be sub-optimal. This is an introduction to a special issue of papers devoted to exploring factors affecting diet and physical activity in adolescents, including food insecure and vulnerable groups.
SettingEight settings including urban, peri-urban and rural across sites from five different low- and middle-income countries.
Design:Focus groups with adolescents and caregivers carried out by trained researchers.
Results:Our results show that adolescents, even in poor settings, know about healthy diet and lifestyles. They want to have energy, feel happy, look good and live longer, but their desire for autonomy, a need to ‘belong’ in their peer group, plus vulnerability to marketing exploiting their aspirations, leads them to make unhealthy choices. They describe significant gender, culture and context-specific barriers. For example, urban adolescents had easy access to energy dense, unhealthy foods bought outside the home, whereas junk foods were only beginning to permeate rural sites. Among adolescents in Indian sites, pressure to excel in exams meant that academic studies were squeezing out physical activity time.
Conclusions:Interventions to improve adolescents’ diets and physical activity levels must therefore address structural and environmental issues and influences in their homes and schools, since it is clear that their food and activity choices are the product of an interacting complex of factors. In the next phase of work, the Transforming Adolescent Lives through Nutrition consortium will employ groups of adolescents, caregivers and local stakeholders in each site to develop interventions to improve adolescent nutritional status.
Market organization and animal genetic resource management: a revealed preference analysis of sheep pricing
- K. Tindano, N. Moula, P. Leroy, A. Traoré, N. Antoine-Moussiaux
-
- Article
- Export citation
-
Farm animal genetic resources are threatened worldwide. Participation in markets, while representing a crucial way out of poverty for many smallholders, affects genetic management choices with associated sustainability concerns. This paper proposes a contextualized study of the interactions between markets and animal genetic resources management, in the case of sheep markets in Ouagadougou, Burkina Faso. It focusses on the organization of marketing chains and the valuation of genetic characteristics by value chain actors. Marketing chain characterization was tackled through semi-structured interviews with 25 exporters and 15 butchers, both specialized in sheep. Moreover, revealed preference methods were applied to analyse the impact of animals’ attributes on market pricing. Data were collected from 338 transactions during three different periods: Eid al-Adha, Christmas and New Year period, and a neutral period. The neutral period is understood as a period not close to any event likely to influence the demand for sheep. The results show that physical characteristics such as live weight, height at withers and coat colour have a strong influence on the animals’ prices. Live weight has also had an increasing marginal impact on price. The different markets (local butcher, feasts, export market, sacrifices) represent distinct demands for genetic characteristics, entailing interesting consequences for animal genetic resource management. Any breeding programme should therefore take this diversity into account to allow this sector to contribute better to a sustainable development of the country.
Local Physics and Star Formation in Galaxies
- Part of
- Adam K. Leroy, Frank Bigiel, Annie Hughes, Eva Schinnerer, Antonio Usero, the PAWS, EMPIRE, and HERACLES Dense Gas Collaborations
-
- Journal:
- Proceedings of the International Astronomical Union / Volume 11 / Issue S315 / August 2015
- Published online by Cambridge University Press:
- 12 September 2016, pp. 175-182
- Print publication:
- August 2015
-
- Article
-
- You have access Access
- Export citation
-
A next main step in understanding star formation is to link the sharp but narrow view of Galactic molecular cloud studies to the wider context accessed by less detail by extragalactic work. In this proceeding, we discuss how new technology and large programs at millimeter wavelengths are improving our ability to access physical conditions in the interstellar medium (ISM) of other galaxies. We highlight results from the multi-line survey of Usero et al. (2015), which measured density sensitive lines across nearby galaxy disks, and two new mapping studies of M51: the high resolution Plateau de Bure Arcsecond Whirlpool Survey (PAWS) and the EMPIRE multi-line mapping survey. These results argue for a context-dependent role for gas density in star formation; that is, gas at a particular density does not appear to form stars in a universal way. They also demonstrate the influence of cloud-scale conditions, especially surface density and the velocity dispersion, in setting the small-scale density distribution and highlight gravitational boundedness as a main driver of the ability of gas to form stars. Beyond these specific results, we argue that ability to gauge detailed physical conditions in the star-forming gas of other galaxies promises major advances that will help unify the fields of Galactic and extragalactic star formation in the next few years.
Chapter Nineteen - Functional and heritable consequences of plant genotype on community composition and ecosystem processes
-
- By Jennifer A. Schweitzer, Department of Ecology and Evolutionary Biology, University of Tennessee, Joseph K. Bailey, Department of Ecology and Evolutionary Biology, University of Tennessee, Dylan G. Fischer, Environmental Studies Program, The Evergreen State College, Carri J. LeRoy, Environmental Studies Program, The Evergreen State College, Thomas G. Whitham, Department of Biological Sciences, Northern Arizona University, Stephen C. Hart, School of Natural Sciences and Sierra Nevada Research Institute, University of California – Merced
- Edited by Takayuki Ohgushi, Kyoto University, Japan, Oswald Schmitz, Yale University, Connecticut, Robert D. Holt, University of Florida
-
- Book:
- Trait-Mediated Indirect Interactions
- Published online:
- 05 February 2013
- Print publication:
- 06 December 2012, pp 371-390
-
- Chapter
- Export citation
-
Summary
Introduction
Foundation species represent excellent model systems for understanding the broad consequences of variation on community and ecosystem processes as they provide a focal resource upon which associated interacting species depend. As foundation species (Dayton 1972; Ellison et al. 2005), trees and other dominant plants often create stable conditions via plant traits that allow dependent communities to assemble regularly and influence ecosystem processes such as net primary productivity (NPP) and soil fertility (i.e., nutrient cycling, via accumulations of leaf or root organic matter or root exudates; Zinke 1962; Zak et al. 1986; Binkley and Giardina 1998; Bartelt-Ryser et al. 2005; Wardle 2006). Recent studies in both terrestrial and aquatic habitats have shown that intraspecific genetic variation (defined at multiple genetic scales, including introgression [movement of genes from one species to another], genotypic diversity [studies manipulating the number of genotypes in a population] and genotypic variation [variation among genotypes]) in foundation plants can have community-wide consequences. Intraspecific variation affects associated vertebrate, arthropod and microbial community composition or activity and ecosystem level processes (recently reviewed in Johnson and Stinchcombe 2007; Hughes et al. 2008; Whitham et al. 2008; Bailey et al. 2009). For example, genetic variation resulting from the introgression of genes from one species to another through the process of hybridization has been shown to have important consequences for associated species, communities and ecosystem processes in multiple hybridizing plant species, including Salix spp., Eucalyptus spp., Quercus spp. and Populus spp. (Fritz et al. 1994; Dungey et al. 2000; Hochwender and Fritz 2004; Ito and Ozaki 2005; Wimp et al. 2005; Tovar-Sanchez and Oyama 2006; Bangert et al. 2008). In the Populus system specifically, recent field and common garden studies have shown that genetic variation across a hybridizing system (P. fremontii, P. angustifolia and their natural F1 and backcross hybrids) results in shifts in plant traits, including secondary chemistry, plant water use and above- and belowground productivity (Fischer et al. 2004; Rehill et al. 2006; Schweitzer et al. 2008a; Lojewski et al. 2009). Whether due directly or indirectly to these plant traits, rates of leaf litter decomposition, total belowground carbon (C) allocation and pools of soil nitrogen (N) and rates of net N mineralization also shift along this genetic gradient (Schweitzer et al. 2004, 2008, b; LeRoy et al. 2006; Whitham et al. 2006; Lojewski et al. 2009; Fischer et al. 2007, 2010).
An Updated View of Giant Molecular Clouds, Gas Flows and Star Formation in M51 with PAWS
- S. E. Meidt, E. Schinnerer, A. Hughes, D. Colombo, J. Pety, S. Garcia-Burillo, A. Leroy, C. L. Dobbs, K. F. Schuster, C. Kramer, G. Dumas, T. Thompson
-
- Journal:
- Proceedings of the International Astronomical Union / Volume 8 / Issue S292 / August 2012
- Published online by Cambridge University Press:
- 21 March 2013, pp. 139-142
- Print publication:
- August 2012
-
- Article
-
- You have access Access
- Export citation
-
We present an overview of the latest results from the PdBI Arcsecond Whirlpool Survey (PAWS, PI: E. Schinnerer), which has mapped CO(1-0) emission in the nearby grand-design spiral galaxy M51 at 40pc resolution. Our data are sensitive to GMCs above 105 M⊙, allowing the construction of the largest GMC catalog to date – containing over 1500 objects – using the CPROPS algorithm (Rosolowsky & Leroy 2006). In the inner disk of M51, the properties of the CO emission show significant variation that can be linked to the dynamical environment in which the molecular gas is located. We find that dynamically distinct regions host clouds with different properties and exhibit different GMC mass spectra, as well as distinct patterns of star formation. To understand how this sensitivity to environment emerges, we consider the role of pressure on GMC stabilization (including shear and star formation feedback-driven turbulence). We suggest that, in the presence of significant external pressure, streaming motions driven by the spiral arm can act to reduce the surface pressure on clouds. The resulting stabilization impacts the global pattern of star formation and can account for the observed non-monotonic radial dependence of the gas depletion time. Our findings have implications for the observed scatter in the standard GMC relations and extragalactic star formation laws.
Chapter Fourteen - From genes to ecosystems
-
- By Joseph K. Bailey, Department of Ecology and Evolutionary Biology, University of Tennessee, Jennifer A. Schweitzer, Department of Ecology and Evolutionary Biology, University of Tennessee, Francisco Úbeda, Department of Ecology and Evolutionary Biology, University of Tennessee, Benjamin M. Fitzpatrick, Department of Ecology and Evolutionary Biology, University of Tennessee, Mark A. Genung, Department of Ecology and Evolutionary Biology, University of Tennessee, Clara C. Pregitzer, Department of Ecology and Evolutionary Biology, University of Tennessee, Matthew Zinkgraf, Department of Biological Sciences, Northern Arizona University, Thomas G. Whitham, Department of Biological Sciences, Northern Arizona University, Arthur Keith, Department of Biological Sciences, Northern Arizona University, Julianne M. O’Reilly-Wapstra, Bradley M. Potts, School of Plant Science, University of Tasmania, Brian J. Rehill, Department of Chemistry, US Naval Academy, Carri J. LeRoy, Environmental Studies Program, The Evergreen State College, Dylan G. Fischer, Environmental Studies Program, The Evergreen State College
- Edited by Glenn R. Iason, Marcel Dicke, Wageningen Universiteit, The Netherlands, Susan E. Hartley, University of York
-
- Book:
- The Ecology of Plant Secondary Metabolites
- Published online:
- 05 August 2012
- Print publication:
- 19 April 2012, pp 269-286
-
- Chapter
- Export citation
-
Summary
Introduction
Relatively little is understood about the extent to which evolution in one species can result in changes to associated communities and ecosystems, the potential mechanisms responsible for those changes (genetic drift, gene flow or natural selection), the phenotypes or candidate genes that may link ecological and evolutionary dynamics, or the role of rapid evolution and feedbacks. However, linking genes and ecosystems in this manner is fundamental to placing community structure and ecosystem function in an evolutionary framework. This is not an easy endeavour as the field of community genetics is multi-disciplinary (Whitham et al., 2006), and ecological and evolutionary dynamics occur at different spatial and temporal scales. Recent reviews show that plant genetic variation can have extended consequences at the community and ecosystem level (extended phenotype; Whitham et al., 2003) affecting arthropod diversity, soil microbial communities, trophic interactions, carbon dynamics and soil nitrogen availability (Whitham et al., 2006; Johnson & Stinchcombe, 2007; Hughes et al., 2008; Bailey et al., 2009a). Its effects are not limited to single systems or even foundation species, but are common across broadly distributed plant and animal systems, and can have effects at the community and ecosystem level of similar magnitude to traditional ecological factors, such as differences among species (Bailey et al., 2009a, b).
Theory in the fields of community genetics (Shuster et al., 2006; Whitham et al., 2006) and co-evolution (Thompson, 2005) also supports the connection between evolutionary and ecological dynamics (Johnson et al., 2009). Multiple investigators argue that community and ecosystem phenotypes represent complex traits related to variation in the fitness consequences of inter-specific indirect genetic effects (IIGEs) (Thompson, 2005; Shuster et al., 2006; Whitham et al., 2006; Tetard-Jones et al., 2007). In their most basic form, IIGEs occur when the genotype of one individual affects the phenotype and fitness of an associated individual of a different species (Moore et al.,1997; Agrawal et al., 2001; Shuster et al., 2006; Wade, 2007). Such interactions are important in the geographic mosaic theory of co-evolution (Thompson, 2005), the development of community heritability (Shuster et al., 2006) and non-additive responses of community structure, biodiversity and ecosystem function (Bailey et al., 2009a). Empirical evidence for the effects of plant genetic variation on communities and ecosystems, paired with growing theoretical models explaining evolutionary mechanisms for these results, provides a solid foundation for understanding how evolutionary processes, such as drift and selection, may affect community structure and ecosystem function.
Hydrodynamic study of a microwave plasma torch
- K. Gadonna, O. Leroy, T. Silva, P. Leprince, C. Boisse-Laporte, L.L. Alves
-
- Journal:
- The European Physical Journal - Applied Physics / Volume 56 / Issue 2 / November 2011
- Published online by Cambridge University Press:
- 28 October 2011, 24008
- Print publication:
- November 2011
-
- Article
- Export citation
-
A hydrodynamic model was developed to simulate the flow and the heat transfer with the gas/plasma system produced by a microwave-driven (500–900 W at 2.45 GHz) axial injection torch, running in atmospheric pressure helium at 3–9 L min−1 input gas flows. The model solves the Navier-Stokes’ equations, including the effect of the plasma upon the momentum and the energy balance, in order to obtain the spatial distributions of the gas velocity and temperature. The model predicts average gas temperatures of 2500–3500 K, in the same range of those obtained by optical measurements. Simulations show that the plasma influences the gas flow path and temperature, promoting an efficient power transfer.
A Radio View of Star Formation in II Zw 40
- M. Koleva, Ph. Prugniel, I. Vauglin, A. Kepley, A. Reines, K. Johnson, A. Leroy, L.M. Walker
-
- Journal:
- European Astronomical Society Publications Series / Volume 48 / 2011
- Published online by Cambridge University Press:
- 11 July 2011, pp. 155-156
- Print publication:
- 2011
-
- Article
- Export citation
-
Star formation in the low mass and low metallicity environments of dwarf galaxies provides important clues about how star formation proceeded in the early universe. To measure the properties of youngest star forming regions – those closest to stellar birth conditions – one needs to use an extinction-free tracer of thermal emission, such as free-free continuum emission in the radio, to penetrate the dust surrounding these regions. We present high sensitivity and high resolution observations of the radio continuum emission in the low metallicity dwarf galaxy II Zw 40 and combine it with HST ACS data and single dish CO(1–0) to gain a more complete picture of star formation in this galaxy.
Contributors
-
- By Rose Teteki Abbey, K. C. Abraham, David Tuesday Adamo, LeRoy H. Aden, Efrain Agosto, Victor Aguilan, Gillian T. W. Ahlgren, Charanjit Kaur AjitSingh, Dorothy B E A Akoto, Giuseppe Alberigo, Daniel E. Albrecht, Ruth Albrecht, Daniel O. Aleshire, Urs Altermatt, Anand Amaladass, Michael Amaladoss, James N. Amanze, Lesley G. Anderson, Thomas C. Anderson, Victor Anderson, Hope S. Antone, María Pilar Aquino, Paula Arai, Victorio Araya Guillén, S. Wesley Ariarajah, Ellen T. Armour, Brett Gregory Armstrong, Atsuhiro Asano, Naim Stifan Ateek, Mahmoud Ayoub, John Alembillah Azumah, Mercedes L. García Bachmann, Irena Backus, J. Wayne Baker, Mieke Bal, Lewis V. Baldwin, William Barbieri, António Barbosa da Silva, David Basinger, Bolaji Olukemi Bateye, Oswald Bayer, Daniel H. Bays, Rosalie Beck, Nancy Elizabeth Bedford, Guy-Thomas Bedouelle, Chorbishop Seely Beggiani, Wolfgang Behringer, Christopher M. Bellitto, Byard Bennett, Harold V. Bennett, Teresa Berger, Miguel A. Bernad, Henley Bernard, Alan E. Bernstein, Jon L. Berquist, Johannes Beutler, Ana María Bidegain, Matthew P. Binkewicz, Jennifer Bird, Joseph Blenkinsopp, Dmytro Bondarenko, Paulo Bonfatti, Riet en Pim Bons-Storm, Jessica A. Boon, Marcus J. Borg, Mark Bosco, Peter C. Bouteneff, François Bovon, William D. Bowman, Paul S. Boyer, David Brakke, Richard E. Brantley, Marcus Braybrooke, Ian Breward, Ênio José da Costa Brito, Jewel Spears Brooker, Johannes Brosseder, Nicholas Canfield Read Brown, Robert F. Brown, Pamela K. Brubaker, Walter Brueggemann, Bishop Colin O. Buchanan, Stanley M. Burgess, Amy Nelson Burnett, J. Patout Burns, David B. Burrell, David Buttrick, James P. Byrd, Lavinia Byrne, Gerado Caetano, Marcos Caldas, Alkiviadis Calivas, William J. Callahan, Salvatore Calomino, Euan K. Cameron, William S. Campbell, Marcelo Ayres Camurça, Daniel F. Caner, Paul E. Capetz, Carlos F. Cardoza-Orlandi, Patrick W. Carey, Barbara Carvill, Hal Cauthron, Subhadra Mitra Channa, Mark D. Chapman, James H. Charlesworth, Kenneth R. Chase, Chen Zemin, Luciano Chianeque, Philip Chia Phin Yin, Francisca H. Chimhanda, Daniel Chiquete, John T. Chirban, Soobin Choi, Robert Choquette, Mita Choudhury, Gerald Christianson, John Chryssavgis, Sejong Chun, Esther Chung-Kim, Charles M. A. Clark, Elizabeth A. Clark, Sathianathan Clarke, Fred Cloud, John B. Cobb, W. Owen Cole, John A Coleman, John J. Collins, Sylvia Collins-Mayo, Paul K. Conkin, Beth A. Conklin, Sean Connolly, Demetrios J. Constantelos, Michael A. Conway, Paula M. Cooey, Austin Cooper, Michael L. Cooper-White, Pamela Cooper-White, L. William Countryman, Sérgio Coutinho, Pamela Couture, Shannon Craigo-Snell, James L. Crenshaw, David Crowner, Humberto Horacio Cucchetti, Lawrence S. Cunningham, Elizabeth Mason Currier, Emmanuel Cutrone, Mary L. Daniel, David D. Daniels, Robert Darden, Rolf Darge, Isaiah Dau, Jeffry C. Davis, Jane Dawson, Valentin Dedji, John W. de Gruchy, Paul DeHart, Wendy J. Deichmann Edwards, Miguel A. De La Torre, George E. Demacopoulos, Thomas de Mayo, Leah DeVun, Beatriz de Vasconcellos Dias, Dennis C. Dickerson, John M. Dillon, Luis Miguel Donatello, Igor Dorfmann-Lazarev, Susanna Drake, Jonathan A. Draper, N. Dreher Martin, Otto Dreydoppel, Angelyn Dries, A. J. Droge, Francis X. D'Sa, Marilyn Dunn, Nicole Wilkinson Duran, Rifaat Ebied, Mark J. Edwards, William H. Edwards, Leonard H. Ehrlich, Nancy L. Eiesland, Martin Elbel, J. Harold Ellens, Stephen Ellingson, Marvin M. Ellison, Robert Ellsberg, Jean Bethke Elshtain, Eldon Jay Epp, Peter C. Erb, Tassilo Erhardt, Maria Erling, Noel Leo Erskine, Gillian R. Evans, Virginia Fabella, Michael A. Fahey, Edward Farley, Margaret A. Farley, Wendy Farley, Robert Fastiggi, Seena Fazel, Duncan S. Ferguson, Helwar Figueroa, Paul Corby Finney, Kyriaki Karidoyanes FitzGerald, Thomas E. FitzGerald, John R. Fitzmier, Marie Therese Flanagan, Sabina Flanagan, Claude Flipo, Ronald B. Flowers, Carole Fontaine, David Ford, Mary Ford, Stephanie A. Ford, Jim Forest, William Franke, Robert M. Franklin, Ruth Franzén, Edward H. Friedman, Samuel Frouisou, Lorelei F. Fuchs, Jojo M. Fung, Inger Furseth, Richard R. Gaillardetz, Brandon Gallaher, China Galland, Mark Galli, Ismael García, Tharscisse Gatwa, Jean-Marie Gaudeul, Luis María Gavilanes del Castillo, Pavel L. Gavrilyuk, Volney P. Gay, Metropolitan Athanasios Geevargis, Kondothra M. George, Mary Gerhart, Simon Gikandi, Maurice Gilbert, Michael J. Gillgannon, Verónica Giménez Beliveau, Terryl Givens, Beth Glazier-McDonald, Philip Gleason, Menghun Goh, Brian Golding, Bishop Hilario M. Gomez, Michelle A. Gonzalez, Donald K. Gorrell, Roy Gottfried, Tamara Grdzelidze, Joel B. Green, Niels Henrik Gregersen, Cristina Grenholm, Herbert Griffiths, Eric W. Gritsch, Erich S. Gruen, Christoffer H. Grundmann, Paul H. Gundani, Jon P. Gunnemann, Petre Guran, Vidar L. Haanes, Jeremiah M. Hackett, Getatchew Haile, Douglas John Hall, Nicholas Hammond, Daphne Hampson, Jehu J. Hanciles, Barry Hankins, Jennifer Haraguchi, Stanley S. Harakas, Anthony John Harding, Conrad L. Harkins, J. William Harmless, Marjory Harper, Amir Harrak, Joel F. Harrington, Mark W. Harris, Susan Ashbrook Harvey, Van A. Harvey, R. Chris Hassel, Jione Havea, Daniel Hawk, Diana L. Hayes, Leslie Hayes, Priscilla Hayner, S. Mark Heim, Simo Heininen, Richard P. Heitzenrater, Eila Helander, David Hempton, Scott H. Hendrix, Jan-Olav Henriksen, Gina Hens-Piazza, Carter Heyward, Nicholas J. Higham, David Hilliard, Norman A. Hjelm, Peter C. Hodgson, Arthur Holder, M. Jan Holton, Dwight N. Hopkins, Ronnie Po-chia Hsia, Po-Ho Huang, James Hudnut-Beumler, Jennifer S. Hughes, Leonard M. Hummel, Mary E. Hunt, Laennec Hurbon, Mark Hutchinson, Susan E. Hylen, Mary Beth Ingham, H. Larry Ingle, Dale T. Irvin, Jon Isaak, Paul John Isaak, Ada María Isasi-Díaz, Hans Raun Iversen, Margaret C. Jacob, Arthur James, Maria Jansdotter-Samuelsson, David Jasper, Werner G. Jeanrond, Renée Jeffery, David Lyle Jeffrey, Theodore W. Jennings, David H. Jensen, Robin Margaret Jensen, David Jobling, Dale A. Johnson, Elizabeth A. Johnson, Maxwell E. Johnson, Sarah Johnson, Mark D. Johnston, F. Stanley Jones, James William Jones, John R. Jones, Alissa Jones Nelson, Inge Jonsson, Jan Joosten, Elizabeth Judd, Mulambya Peggy Kabonde, Robert Kaggwa, Sylvester Kahakwa, Isaac Kalimi, Ogbu U. Kalu, Eunice Kamaara, Wayne C. Kannaday, Musimbi Kanyoro, Veli-Matti Kärkkäinen, Frank Kaufmann, Léon Nguapitshi Kayongo, Richard Kearney, Alice A. Keefe, Ralph Keen, Catherine Keller, Anthony J. Kelly, Karen Kennelly, Kathi Lynn Kern, Fergus Kerr, Edward Kessler, George Kilcourse, Heup Young Kim, Kim Sung-Hae, Kim Yong-Bock, Kim Yung Suk, Richard King, Thomas M. King, Robert M. Kingdon, Ross Kinsler, Hans G. Kippenberg, Cheryl A. Kirk-Duggan, Clifton Kirkpatrick, Leonid Kishkovsky, Nadieszda Kizenko, Jeffrey Klaiber, Hans-Josef Klauck, Sidney Knight, Samuel Kobia, Robert Kolb, Karla Ann Koll, Heikki Kotila, Donald Kraybill, Philip D. W. Krey, Yves Krumenacker, Jeffrey Kah-Jin Kuan, Simanga R. Kumalo, Peter Kuzmic, Simon Shui-Man Kwan, Kwok Pui-lan, André LaCocque, Stephen E. Lahey, John Tsz Pang Lai, Emiel Lamberts, Armando Lampe, Craig Lampe, Beverly J. Lanzetta, Eve LaPlante, Lizette Larson-Miller, Ariel Bybee Laughton, Leonard Lawlor, Bentley Layton, Robin A. Leaver, Karen Lebacqz, Archie Chi Chung Lee, Marilyn J. Legge, Hervé LeGrand, D. L. LeMahieu, Raymond Lemieux, Bill J. Leonard, Ellen M. Leonard, Outi Leppä, Jean Lesaulnier, Nantawan Boonprasat Lewis, Henrietta Leyser, Alexei Lidov, Bernard Lightman, Paul Chang-Ha Lim, Carter Lindberg, Mark R. Lindsay, James R. Linville, James C. Livingston, Ann Loades, David Loades, Jean-Claude Loba-Mkole, Lo Lung Kwong, Wati Longchar, Eleazar López, David W. Lotz, Andrew Louth, Robin W. Lovin, William Luis, Frank D. Macchia, Diarmaid N. J. MacCulloch, Kirk R. MacGregor, Marjory A. MacLean, Donald MacLeod, Tomas S. Maddela, Inge Mager, Laurenti Magesa, David G. Maillu, Fortunato Mallimaci, Philip Mamalakis, Kä Mana, Ukachukwu Chris Manus, Herbert Robinson Marbury, Reuel Norman Marigza, Jacqueline Mariña, Antti Marjanen, Luiz C. L. Marques, Madipoane Masenya (ngwan'a Mphahlele), Caleb J. D. Maskell, Steve Mason, Thomas Massaro, Fernando Matamoros Ponce, András Máté-Tóth, Odair Pedroso Mateus, Dinis Matsolo, Fumitaka Matsuoka, John D'Arcy May, Yelena Mazour-Matusevich, Theodore Mbazumutima, John S. McClure, Christian McConnell, Lee Martin McDonald, Gary B. McGee, Thomas McGowan, Alister E. McGrath, Richard J. McGregor, John A. McGuckin, Maud Burnett McInerney, Elsie Anne McKee, Mary B. McKinley, James F. McMillan, Ernan McMullin, Kathleen E. McVey, M. Douglas Meeks, Monica Jyotsna Melanchthon, Ilie Melniciuc-Puica, Everett Mendoza, Raymond A. Mentzer, William W. Menzies, Ina Merdjanova, Franziska Metzger, Constant J. Mews, Marvin Meyer, Carol Meyers, Vasile Mihoc, Gunner Bjerg Mikkelsen, Maria Inêz de Castro Millen, Clyde Lee Miller, Bonnie J. Miller-McLemore, Alexander Mirkovic, Paul Misner, Nozomu Miyahira, R. W. L. Moberly, Gerald Moede, Aloo Osotsi Mojola, Sunanda Mongia, Rebeca Montemayor, James Moore, Roger E. Moore, Craig E. Morrison O.Carm, Jeffry H. Morrison, Keith Morrison, Wilson J. Moses, Tefetso Henry Mothibe, Mokgethi Motlhabi, Fulata Moyo, Henry Mugabe, Jesse Ndwiga Kanyua Mugambi, Peggy Mulambya-Kabonde, Robert Bruce Mullin, Pamela Mullins Reaves, Saskia Murk Jansen, Heleen L. Murre-Van den Berg, Augustine Musopole, Isaac M. T. Mwase, Philomena Mwaura, Cecilia Nahnfeldt, Anne Nasimiyu Wasike, Carmiña Navia Velasco, Thulani Ndlazi, Alexander Negrov, James B. Nelson, David G. Newcombe, Carol Newsom, Helen J. Nicholson, George W. E. Nickelsburg, Tatyana Nikolskaya, Damayanthi M. A. Niles, Bertil Nilsson, Nyambura Njoroge, Fidelis Nkomazana, Mary Beth Norton, Christian Nottmeier, Sonene Nyawo, Anthère Nzabatsinda, Edward T. Oakes, Gerald O'Collins, Daniel O'Connell, David W. Odell-Scott, Mercy Amba Oduyoye, Kathleen O'Grady, Oyeronke Olajubu, Thomas O'Loughlin, Dennis T. Olson, J. Steven O'Malley, Cephas N. Omenyo, Muriel Orevillo-Montenegro, César Augusto Ornellas Ramos, Agbonkhianmeghe E. Orobator, Kenan B. Osborne, Carolyn Osiek, Javier Otaola Montagne, Douglas F. Ottati, Anna May Say Pa, Irina Paert, Jerry G. Pankhurst, Aristotle Papanikolaou, Samuele F. Pardini, Stefano Parenti, Peter Paris, Sung Bae Park, Cristián G. Parker, Raquel Pastor, Joseph Pathrapankal, Daniel Patte, W. Brown Patterson, Clive Pearson, Keith F. Pecklers, Nancy Cardoso Pereira, David Horace Perkins, Pheme Perkins, Edward N. Peters, Rebecca Todd Peters, Bishop Yeznik Petrossian, Raymond Pfister, Peter C. Phan, Isabel Apawo Phiri, William S. F. Pickering, Derrick G. Pitard, William Elvis Plata, Zlatko Plese, John Plummer, James Newton Poling, Ronald Popivchak, Andrew Porter, Ute Possekel, James M. Powell, Enos Das Pradhan, Devadasan Premnath, Jaime Adrían Prieto Valladares, Anne Primavesi, Randall Prior, María Alicia Puente Lutteroth, Eduardo Guzmão Quadros, Albert Rabil, Laurent William Ramambason, Apolonio M. Ranche, Vololona Randriamanantena Andriamitandrina, Lawrence R. Rast, Paul L. Redditt, Adele Reinhartz, Rolf Rendtorff, Pål Repstad, James N. Rhodes, John K. Riches, Joerg Rieger, Sharon H. Ringe, Sandra Rios, Tyler Roberts, David M. Robinson, James M. Robinson, Joanne Maguire Robinson, Richard A. H. Robinson, Roy R. Robson, Jack B. Rogers, Maria Roginska, Sidney Rooy, Rev. Garnett Roper, Maria José Fontelas Rosado-Nunes, Andrew C. Ross, Stefan Rossbach, François Rossier, John D. Roth, John K. Roth, Phillip Rothwell, Richard E. Rubenstein, Rosemary Radford Ruether, Markku Ruotsila, John E. Rybolt, Risto Saarinen, John Saillant, Juan Sanchez, Wagner Lopes Sanchez, Hugo N. Santos, Gerhard Sauter, Gloria L. Schaab, Sandra M. Schneiders, Quentin J. Schultze, Fernando F. Segovia, Turid Karlsen Seim, Carsten Selch Jensen, Alan P. F. Sell, Frank C. Senn, Kent Davis Sensenig, Damían Setton, Bal Krishna Sharma, Carolyn J. Sharp, Thomas Sheehan, N. Gerald Shenk, Christian Sheppard, Charles Sherlock, Tabona Shoko, Walter B. Shurden, Marguerite Shuster, B. Mark Sietsema, Batara Sihombing, Neil Silberman, Clodomiro Siller, Samuel Silva-Gotay, Heikki Silvet, John K. Simmons, Hagith Sivan, James C. Skedros, Abraham Smith, Ashley A. Smith, Ted A. Smith, Daud Soesilo, Pia Søltoft, Choan-Seng (C. S.) Song, Kathryn Spink, Bryan Spinks, Eric O. Springsted, Nicolas Standaert, Brian Stanley, Glen H. Stassen, Karel Steenbrink, Stephen J. Stein, Andrea Sterk, Gregory E. Sterling, Columba Stewart, Jacques Stewart, Robert B. Stewart, Cynthia Stokes Brown, Ken Stone, Anne Stott, Elizabeth Stuart, Monya Stubbs, Marjorie Hewitt Suchocki, David Kwang-sun Suh, Scott W. Sunquist, Keith Suter, Douglas Sweeney, Charles H. Talbert, Shawqi N. Talia, Elsa Tamez, Joseph B. Tamney, Jonathan Y. Tan, Yak-Hwee Tan, Kathryn Tanner, Feiya Tao, Elizabeth S. Tapia, Aquiline Tarimo, Claire Taylor, Mark Lewis Taylor, Bishop Abba Samuel Wolde Tekestebirhan, Eugene TeSelle, M. Thomas Thangaraj, David R. Thomas, Andrew Thornley, Scott Thumma, Marcelo Timotheo da Costa, George E. “Tink” Tinker, Ola Tjørhom, Karen Jo Torjesen, Iain R. Torrance, Fernando Torres-Londoño, Archbishop Demetrios [Trakatellis], Marit Trelstad, Christine Trevett, Phyllis Trible, Johannes Tromp, Paul Turner, Robert G. Tuttle, Archbishop Desmond Tutu, Peter Tyler, Anders Tyrberg, Justin Ukpong, Javier Ulloa, Camillus Umoh, Kristi Upson-Saia, Martina Urban, Monica Uribe, Elochukwu Eugene Uzukwu, Richard Vaggione, Gabriel Vahanian, Paul Valliere, T. J. Van Bavel, Steven Vanderputten, Peter Van der Veer, Huub Van de Sandt, Louis Van Tongeren, Luke A. Veronis, Noel Villalba, Ramón Vinke, Tim Vivian, David Voas, Elena Volkova, Katharina von Kellenbach, Elina Vuola, Timothy Wadkins, Elaine M. Wainwright, Randi Jones Walker, Dewey D. Wallace, Jerry Walls, Michael J. Walsh, Philip Walters, Janet Walton, Jonathan L. Walton, Wang Xiaochao, Patricia A. Ward, David Harrington Watt, Herold D. Weiss, Laurence L. Welborn, Sharon D. Welch, Timothy Wengert, Traci C. West, Merold Westphal, David Wetherell, Barbara Wheeler, Carolinne White, Jean-Paul Wiest, Frans Wijsen, Terry L. Wilder, Felix Wilfred, Rebecca Wilkin, Daniel H. Williams, D. Newell Williams, Michael A. Williams, Vincent L. Wimbush, Gabriele Winkler, Anders Winroth, Lauri Emílio Wirth, James A. Wiseman, Ebba Witt-Brattström, Teofil Wojciechowski, John Wolffe, Kenman L. Wong, Wong Wai Ching, Linda Woodhead, Wendy M. Wright, Rose Wu, Keith E. Yandell, Gale A. Yee, Viktor Yelensky, Yeo Khiok-Khng, Gustav K. K. Yeung, Angela Yiu, Amos Yong, Yong Ting Jin, You Bin, Youhanna Nessim Youssef, Eliana Yunes, Robert Michael Zaller, Valarie H. Ziegler, Barbara Brown Zikmund, Joyce Ann Zimmerman, Aurora Zlotnik, Zhuo Xinping
- Edited by Daniel Patte, Vanderbilt University, Tennessee
-
- Book:
- The Cambridge Dictionary of Christianity
- Published online:
- 05 August 2012
- Print publication:
- 20 September 2010, pp xi-xliv
-
- Chapter
- Export citation
RINGS OVER WHICH CYCLICS ARE DIRECT SUMS OF PROJECTIVE AND CS OR NOETHERIAN*
- C. J. HOLSTON, S. K. JAIN, A. LEROY
-
- Journal:
- Glasgow Mathematical Journal / Volume 52 / Issue A / July 2010
- Published online by Cambridge University Press:
- 24 June 2010, pp. 103-110
- Print publication:
- July 2010
-
- Article
-
- You have access Access
- Export citation
-
R is called a right WV-ring if each simple right R-module is injective relative to proper cyclics. If R is a right WV-ring, then R is right uniform or a right V-ring. It is shown that a right WV-ring R is right noetherian if and only if each right cyclic module is a direct sum of a projective module and a CS (complements are summands, a.k.a. ‘extending modules’) or noetherian module. For a finitely generated module M with projective socle over a V-ring R such that every subfactor of M is a direct sum of a projective module and a CS or noetherian module, we show M = X ⊕ T, where X is semisimple and T is noetherian with zero socle. In the case where M = R, we get R = S ⊕ T, where S is a semisimple artinian ring and T is a direct sum of right noetherian simple rings with zero socle. In addition, if R is a von Neumann regular ring, then it is semisimple artinian.
3 - A community and ecosystem genetics approach to conservation biology and management
-
- By Thomas G. Whitham, Northern Arizona University, Catherine A. Gehring, Northern Arizona University, Luke M. Evans, Northern Arizona University, Carri J. LeRoy, The Evergreen State College, Randy K. Bangert, Idaho State University, Jennifer A. Schweitzer, University of Tennessee, Gerard J. Allan, Northern Arizona University, Robert C. Barbour, University of Tasmania, Dylan G. Fischer, The Evergreen State College, Bradley M. Potts, University of Tasmania, Joseph K. Bailey, Northern Arizona University
- Edited by J. Andrew DeWoody, Purdue University, Indiana, John W. Bickham, Purdue University, Indiana, Charles H. Michler, Purdue University, Indiana, Krista M. Nichols, Purdue University, Indiana, Gene E. Rhodes, Purdue University, Indiana, Keith E. Woeste, Purdue University, Indiana
-
- Book:
- Molecular Approaches in Natural Resource Conservation and Management
- Published online:
- 05 July 2014
- Print publication:
- 14 June 2010, pp 50-73
-
- Chapter
- Export citation
-
Summary
INTRODUCTION
The emerging field of community and ecosystem genetics has so far focused on how the genetic variation in one species can influence the composition of associated communities and ecosystem processes such as decomposition (see definitions in Table 3–1; reviews by Whitham et al. 2003, 2006; Johnson & Stinchcombe 2007; Hughes et al. 2008). A key component of this approach has been an emphasis on understanding how the genetics of foundation plant species influence a much larger community. It is reasoned that because foundation species structure their ecosystems by creating locally stable conditions and provide specific resources for diverse organisms (Dayton 1972; Ellison et al. 2005), the genetics of these species as “community drivers” are most important to understand and most likely to have cascading ecological and evolutionary effects throughout an ecosystem (Whitham et al. 2006). For example, when a foundation species’ genotype influences the relative fitness of other species, it constitutes an indirect genetic interaction (Shuster et al. 2006), and when these interactions change species composition and abundance among individual tree genotypes, they result in individual genotypes having distinct community and ecosystem phenotypes. Thus, in addition to an individual genotype having the “traditional” phenotype that population geneticists typically consider as the expression of a trait at the individual and population level, community geneticists must also consider higher-level phenotypes at the community and ecosystem level. The predictability of phenotypes at levels higher than the population can be quantified as community heritability (i.e., the tendency for related individuals to support similar communities of organisms and ecosystem processes; Whitham et al. 2003, 2006; Shuster et al. 2006).
The Spitzer spectroscopic survey of the Small Magellanic Cloud: polycyclic aromatic hydrocarbon emission from SMC star-forming regions
- Karin M. Sandstrom, Alberto D. Bolatto, Snežana Stanimirović, J. D. T. Smith, Jacco Th. van Loon, Adam K. Leroy
-
- Journal:
- Proceedings of the International Astronomical Union / Volume 4 / Issue S256 / July 2008
- Published online by Cambridge University Press:
- 01 July 2008, pp. 160-165
- Print publication:
- July 2008
-
- Article
-
- You have access Access
- Export citation
-
Because of its proximity, the Small Magellanic Cloud provides a unique opportunity to map the polycyclic aromatic hydrocarbon (PAH) emission from photo-dissociation regions (PDRs) in a low-metallicity (12 + log(O/H) ~ 8) galaxy at high spatial resolution in order to learn about their abundance and physical state. We present mid-IR spectral mapping observations of star-forming regions in the Small Magellanic Cloud obtained as part of the Spitzer Spectroscopic Survey of the SMC (S4MC) project. These observations allow us to map the distribution of PAH emission in these regions and the measure the variation of PAH band strengths with local physical conditions. In these proceedings we discuss preliminary results on the physical state of the PAHs, in particular their ionization fraction.
Managing Incidental Findings in Human Subjects Research: Analysis and Recommendations
- Susan M. Wolf, Frances P. Lawrenz, Charles A. Nelson, Jeffrey P. Kahn, Mildred K. Cho, Ellen Wright Clayton, Joel G. Fletcher, Michael K. Georgieff, Dale Hammerschmidt, Kathy Hudson, Judy Illes, Vivek Kapur, Moira A. Keane, Barbara A. Koenig, Bonnie S. LeRoy, Elizabeth G. McFarland, Jordan Paradise, Lisa S. Parker, Sharon F. Terry, Brian Van Ness, Benjamin S. Wilfond
-
- Journal:
- Journal of Law, Medicine & Ethics / Volume 36 / Issue 2 / Summer 2008
- Published online by Cambridge University Press:
- 01 January 2021, pp. 219-248
- Print publication:
- Summer 2008
-
- Article
- Export citation
-
Researchers, institutional review boards (IRBs), participants in human subjects research, and their families face an important but largely neglected problem — how should incidental findings (IFs) be managed in human subjects research. If researchers unexpectedly stumble upon information of potential health or reproductive significance, should they seek expert evaluation, contact the participant’s physician, tell the research participant, or respond with some combination? What should consent forms and the entire consent process say about how IFs will be handled in research? What should IRBs require?
The state of molecular gas in the Small Magellanic Cloud
- Adam K. Leroy, Alberto D. Bolatto, Erik Rosolowsky, Snežana Stanimirović, Norikazu Mizuno, Caroline Bot, Frank Israel, Fabian Walter, Leo Blitz
-
- Journal:
- Proceedings of the International Astronomical Union / Volume 4 / Issue S256 / July 2008
- Published online by Cambridge University Press:
- 01 July 2008, pp. 154-159
- Print publication:
- July 2008
-
- Article
-
- You have access Access
- Export citation
-
We compare the resolved properties of giant molecular clouds (GMCs) in the Small Magellanic Cloud (SMC) and other low mass galaxies to those in more massive spirals. When measured using CO line emission, differences among the various populations of GMCs are fairly small. We contrast this result with the view afforded by dust emission in the Small Magellanic Cloud. Comparing temperature-corrected dust opacity to the distribution of H i suggests extended envelopes of CO-free H2, implying that CO traces only the highest density H2 in the SMC. Including this CO-free H2, the gas depletion time, H2-to-H i ratio, and H2-to-stellar mass/light ratio in the SMC are all typical of those found in more massive irregular galaxies.
Early results from the SAGE-SMC Spitzer legacy
- Karl D. Gordon, M. Meixner, R. D. Blum, W. Reach, B. A. Whitney, J. Harris, R. Indebetouw, A. D. Bolatto, J.-P. Bernard, M. Sewilo, B. L. Babler, M. Block, C. Bot, S. Bracker, L. Carlson, E. Churchwell, G. C. Clayton, M. Cohen, C. W. Engelbracht, Y. Fukui, V. Gorjian, S. Hony, J. L. Hora, F. Israel, A. Kawamura, A. K. Leroy, A. Li, S. Madden, A. R. Marble, F. Markwick-Kemper, M. Meade, K. A. Misselt, A. Mizuno, N. Mizuno, E. Muller, J. M. Oliveira, K. Olsen, T. Onishi, R. Paladini, D. Paradis, S. Points, T. Robitaille, D. Rubin, K. M. Sandstrom, S. Sato, H. Shibai, J. D. Simon, L. J. Smith, S. Srinivasan, A. G. G. M. Tielens, U. P. Vijh, S. van Dyk, J. Th. van Loon, K. Volk, D. Zaritsky
-
- Journal:
- Proceedings of the International Astronomical Union / Volume 4 / Issue S256 / July 2008
- Published online by Cambridge University Press:
- 01 July 2008, pp. 184-188
- Print publication:
- July 2008
-
- Article
-
- You have access Access
- Export citation
-
Early results from the SAGE-SMC (Surveying the Agents of Galaxy Evolution in the tidally-disrupted, low-metallicity Small Magellanic Cloud) Spitzer legacy program are presented. These early results concentrate on the SAGE-SMC MIPS observations of the SMC Tail region. This region is the high H i column density portion of the Magellanic Bridge adjacent to the SMC Wing. We detect infrared dust emission and measure the gas-to-dust ratio in the SMC Tail and find it similar to that of the SMC Body. In addition, we find two embedded cluster regions that are resolved into multiple sources at all MIPS wavelengths.