Hostname: page-component-76fb5796d-r6qrq Total loading time: 0 Render date: 2024-04-25T21:05:16.307Z Has data issue: false hasContentIssue false

First results of the Southern Open Cluster Study

Published online by Cambridge University Press:  18 January 2010

K. Kinemuchi
Affiliation:
Departamento de Astronomía, Universidad de Concepción, Concepción, Chile email: kkinemuchi@astro-udec.cl, dgeisler@astro-udec.cl, fmauro@astro-udec.cl Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611, USA email: kinemuchi@astro.ufl.edu, ata@astro.ufl.edu
A. Sarajedini
Affiliation:
Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611, USA email: kinemuchi@astro.ufl.edu, ata@astro.ufl.edu
D. Geisler
Affiliation:
Departamento de Astronomía, Universidad de Concepción, Concepción, Chile email: kkinemuchi@astro-udec.cl, dgeisler@astro-udec.cl, fmauro@astro-udec.cl
F. Mauro
Affiliation:
Departamento de Astronomía, Universidad de Concepción, Concepción, Chile email: kkinemuchi@astro-udec.cl, dgeisler@astro-udec.cl, fmauro@astro-udec.cl
G. Carraro
Affiliation:
European Southern Observatory email: gcarraro@eso.org
S. Kafka
Affiliation:
SSC/Caltech, Pasadena, CA 91125, USA email: stella@caltech.edu
E. Jeffery
Affiliation:
Department of Astronomy, University of Texas at Austin, Austin, TX 78712, USA email: ejeffery@astro.as.utexas.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Galactic open clusters are excellent laboratories to study stellar populations that are coeval and have a common chemical composition. These clusters allow for the investigation of stellar and chemical abundance evolution, binary star systems, mass and luminosity functions, Galactic metallicity gradient, and disk structure, among other things. The Southern Open Cluster Study (socs) is a database of a select set of 24 open clusters with a broad range of ages and metallicities. It is an extension of the northern WIYN Open Cluster Study (wocs). The main goal of both studies is to obtain comprehensive photometric, spectroscopic, and astrometric information of these key open clusters. Here, we provide an overview of the socs survey and present results of the wide-field photometry on two socs clusters, NGC 3532 and Tombaugh 2.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

Frinchaboy, P. M. & Nielsen, D. 2008, in: Vesperini, E., Giersz, M. & Sills, A. (eds.), Dynamical Evolution of Dense Stellar Systems, Proc. IAU Symp. 246, p. 109Google Scholar
Mathieu, R. D. 2000, in: Pallavicini, R., Micela, G., & Sciortino, S. (eds.), Stellar Clusters and Associations: Convection, Rotation, and Dynamos, ASP Conf. Ser., 198, p. 517, San Francisco: ASPGoogle Scholar
Robitaille, T. P., Whitney, B. A., Indebetouw, R., & Wood, K. 2007, ApJS, 169, 328CrossRefGoogle Scholar
Sarajedini, A., Mathieu, R. D., & Platais, I. 2003, in: Oswalt, T. D. (ed.), The Future of Small Telescopes In The New Millennium. III. Science in the Shadows of Giants, ASSL, 289, 257Google Scholar
Stetson, P. B. 1987, PASP, 99, 191CrossRefGoogle Scholar
Stetson, P. B. 1994, PASP, 106, 250CrossRefGoogle Scholar