There is a relative lack of research, targeted models and tools to manage beaches in estuaries and bays (BEBs). Many estuaries and bays have been highly modified and urbanised, for example port developments and coastal revetments. This paper outlines the complications and opportunities for conserving and managing BEBs in modified estuaries. To do this, we focus on eight diverse case studies from North and South America, Asia, Europe, Africa and Australia combined with the broader global literature. Our key findings are as follows: (1) BEBs are diverse and exist under a great variety of tide and wave conditions that differentiate them from open-coast beaches; (2) BEBs often lack statutory protection and many have already been sacrificed to development; (3) BEBs lack specific management tools and are often managed using tools developed for open-coast beaches; and (4) BEBs have the potential to become important in “nature-based” management solutions. We set the future research agenda for BEBs, which should include broadening research to include greater diversity of BEBs than in the past, standardising monitoring techniques, including the development of global databases using citizen science and developing specific management tools for BEBs. We must recognise BEBs as unique coastal features and develop the required fundamental knowledge and tools to effectively manage them, so they can continue providing their unique ecosystem services.

We investigate the diversity in the sizes and average surface densities of the neutral atomic hydrogen (H i) gas discs in $\sim$280 nearby galaxies detected by the Widefield ASKAP L-band Legacy All-sky Blind Survey (WALLABY). We combine the uniformly observed, interferometric H i data from pilot observations of the Hydra cluster and NGC 4636 group fields with photometry measured from ultraviolet, optical, and near-infrared imaging surveys to investigate the interplay between stellar structure, star formation, and H i structural parameters. We quantify the H i structure by the size of the H i relative to the optical disc and the average H i surface density measured using effective and isodensity radii. For galaxies resolved by $>$$1.3$ beams, we find that galaxies with higher stellar masses and stellar surface densities tend to have less extended H i discs and lower H i surface densities: the isodensity H i structural parameters show a weak negative dependence on stellar mass and stellar mass surface density. These trends strengthen when we limit our sample to galaxies resolved by $>$2 beams. We find that galaxies with higher H i surface densities and more extended H i discs tend to be more star forming: the isodensity H i structural parameters have stronger correlations with star formation. Normalising the H i disc size by the optical effective radius (instead of the isophotal radius) produces positive correlations with stellar masses and stellar surface densities and removes the correlations with star formation. This is due to the effective and isodensity H i radii increasing with mass at similar rates while, in the optical, the effective radius increases slower than the isophotal radius. Our results are in qualitative agreement with previous studies and demonstrate that with WALLABY we can begin to bridge the gap between small galaxy samples with high spatial resolution H i data and large, statistical studies using spatially unresolved, single-dish data.

We present the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) Pilot Phase I Hi kinematic models. This first data release consists of Hi observations of three fields in the direction of the Hydra and Norma clusters, and the NGC 4636 galaxy group. In this paper, we describe how we generate and publicly release flat-disk tilted-ring kinematic models for 109/592 unique Hi detections in these fields. The modelling method adopted here—which we call the WALLABY Kinematic Analysis Proto-Pipeline (WKAPP) and for which the corresponding scripts are also publicly available—consists of combining results from the homogeneous application of the FAT and 3DBarolo algorithms to the subset of 209 detections with sufficient resolution and $S/N$ in order to generate optimised model parameters and uncertainties. The 109 models presented here tend to be gas rich detections resolved by at least 3–4 synthesised beams across their major axes, but there is no obvious environmental bias in the modelling. The data release described here is the first step towards the derivation of similar products for thousands of spatially resolved WALLABY detections via a dedicated kinematic pipeline. Such a large publicly available and homogeneously analysed dataset will be a powerful legacy product that that will enable a wide range of scientific studies.

Many books have been written about the incorporation of the Caribbean region, South Asia, Africa and Latin America into the global economy. Remarkably, few have dealt with Island Southeast Asia or Maritime Southeast Asia as a macro-region. For the Caribbean nations, it has been amply discussed how the legacies of the plantation economies consisted of meagre economic growth and massive unemployment. Conversely, scant attention has been given to the question how societies in Island Southeast Asia were turned into providers of cheap commodities and how this impacted their long-term development prospects. This silence is even more remarkable considering some striking parallels with Caribbean socio-economic trajectories. Today, emigration of millions is the fate of Island Southeast Asia, as it is for the Caribbean region. To break the silence and to invite further discussion I wrote The Making of a Periphery: How Island Southeast Asia Became a Mass Exporter. After reading the review by Dr Aguilar on this book in a previous issue of this journal, I felt that it could be worthwhile to highlight some of the main points of my argument about the peripheral integration of Island Southeast Asia in the global economy. I am grateful to the editors of the International Journal of Asian Studies for granting me the opportunity to do so.

At least half of the local galaxies reside in galaxy groups, which indicates that the group is the common environment where galaxies evolve. Therefore, it is important to probe how significantly galaxies are affected by group environmental processes, in order to obtain a better understanding of galaxy evolution. We carried out a new CO imaging survey for 31 galaxies in the IC 1459 and NGC 4636 groups, using the Atacama Compact Array, to study the effect of the group environment on the molecular gas properties and the star formation activity. With our resolved CO data, combined with high-resolution H i images, we find asymmetric CO and H i distributions in the group galaxies. Compared to isolated galaxies, group members have relatively low molecular gas fraction and low star formation rate. These results suggest that the group environment can change the properties of cold gas components and star formation in group galaxies.

Over the past 600 years, commodity frontiers – processes and sites of the incorporation of resources into the expanding capitalist world economy – have absorbed ever more land, ever more labour and ever more natural assets. In this paper, we claim that studying the global history of capitalism through the lens of commodity frontiers and using commodity regimes as an analytical framework is crucial to understanding the origins and nature of capitalism, and thus the modern world. We argue that commodity frontiers identify capitalism as a process rooted in a profound restructuring of the countryside and nature. They connect processes of extraction and exchange with degradation, adaptation and resistance in rural peripheries. To account for the enormous variety of actors and places involved in this history is a critical challenge in the social sciences, and one to which global history can contribute crucial insights.

This rejoinder is part of the round table discussion on the book The Making of a Periphery: How Island Southeast Asia Became a Mass Exporter of Labor. It pays tribute to the development economist and Nobel Prize winner Arthur W. Lewis, who studied the predicaments of plantation societies. The rejoinder addresses critical observations made about the above-mentioned book by Elise van Nederveen Meerkerk, Pim de Zwart, Corey Ross, and Alberto Alonso-Fradejas. It underscores the importance of the role of demography and long histories of labour coercion to explain processes of peripheralization and mass emigration. It also points out the limits of classical development economics, namely a relative neglect of the ecological damage attending plantation exploitation. The commodity frontier approach is suggested as a way to address this shortcoming.

The geographical term “Southeast Asia” dates from the 1930s, and came to denote a topic for academic studies in the early days of the Cold War. As such, it includes Vietnam, Cambodia, Laos, Indochina, Thailand, Myanmar, Malaysia, Brunei, and the Philippines. Southeast Asia has become thoroughly incorporated in the global economy over the past 150 years; first, as a producer of commodities, and later, as a supplier of cheap garments and electronic components. Under Dutch colonialism and British hegemony—the latter established by the conquest of Burma and the imposition of free trade on Siam and the Philippines in the 1850s—Southeast Asia was turned into a key provider of commodities for the industrializing countries. During high colonialism, from 1870 to 1930, the region became increasingly intertwined, via Singapore as the central port and through the role of mainland Southeast Asia as the rice basket for the plantations of maritime Southeast Asia. After the Second World War, the region was the world's most violent frontier of containment for communist expansion. In recent decades, Southeast Asia has become integrated in global commodity chains as a producer of cheap industrial goods, often as a subcontractor for more advanced economies, such as those of Hong Kong, Korea, Taiwan, and later on, Southeast China.

Currently, 25-30% of Obsessive-compulsive disorder (OCD) patients are considered to be resistant to conventional therapies (cognitive-behavioral therapy and medications including selective inhibitors of reuptake of serotonin and clomipramine). Among alternative therapeutic strategies for theses refractory patients, repetitive Transcranial Magnetic Stimulation (rTMS) has been proposed (Greenberg et al., 1997). Few regions were choice for OCD patients and one of them could be a promising target: the Supplementary Motor Area (SMA). The aim of this project focuses on evaluate the SMA as a promising region to treat OCD patients. Forty patients were include in this double blind study, each received 20 session of rTMS (1 session / day) for 4 weeks with active or sham coil. rTMS parameters consisted of 1500 pulses/d, at 1 Hz, 5 trains of 5 min with an interval inter- stimulus of 2 min and 100% of motor threshold. To localize the SMA, neuronavigation was based on anatomical Magnetic Resonance Imaging (MRI) using Brainsight software. The therapeutic effect of rTMS will be assessed through a psychological evaluation and a task performed in functional MRI, before and after therapeutic: The Eriksen’s task. Its objective is to evaluate cerebral metabolism’s modifications during a simple task likely to recruit the error detection system implicating the Anterior Cingulate Cortex without inducing obsessive-compulsive symptoms. This modification were correlated with clinical and cognitive assessment and behavioral results of the Eriksen task

The Square Kilometre Array (SKA) is a planned large radio interferometer designed to operate over a wide range of frequencies, and with an order of magnitude greater sensitivity and survey speed than any current radio telescope. The SKA will address many important topics in astronomy, ranging from planet formation to distant galaxies. However, in this work, we consider the perspective of the SKA as a facility for studying physics. We review four areas in which the SKA is expected to make major contributions to our understanding of fundamental physics: cosmic dawn and reionisation; gravity and gravitational radiation; cosmology and dark energy; and dark matter and astroparticle physics. These discussions demonstrate that the SKA will be a spectacular physics machine, which will provide many new breakthroughs and novel insights on matter, energy, and spacetime.