Export opportunities: women workers organising in the Philippine garments industry

Transnational production arrangements have been widely argued to lessen the organising capacities of industrial workers, none more so than in the case of women workers in 'export' or 'world market' factories in developing countries. This thesis contests this assertion by showing that women workers' ability to form enterprise unions in the Philippine garments industry are enhanced by transnational production arrangements involving an overseas market. Specifically, the thesis demonstrates that, in order to meet the quality and delivery requirements of overseas buyers and contractors, local owners and/or production managers are forced to routinely keep more production in-house in order to exert more direct controls over the work processes of their women sewers. By thereby limiting the amount of local subcontracting which is done, women workers are agglomerated in larger numbers in the one place and, consequently, their capacities to engage in collective action - as indicated by the establishment of enterprise unions - is markedly increased. Empirically, the argument of the thesis draws on a 'multiple-case' study of sixty-five garment-making establishments located in and around Manila. The study involved interviews with owners, production managers and/or trade union officials about the local subcontracting practices of their establishments. The conclusions drawn about the links between export production and enhanced labour organising capacities at the enterprise level are corroborated by the 'commodity chain' literature on industrial deepening in the international garments industry and the status of the Philippine industry in this regard. But rather than think simply in terms of industrial deepening, this thesis is concerned with the impacts of exporting on class processes. Theoretically, the thesis thus draws on the Marxist view that capitalist development entails changes in the social form of labour, through the real subsumption of labour. But, whereas Marx linked the real subsumption of labour to greater capitalist controls over the labour process, in this thesis the real subsumption of labour is also tied to concomitant changes in the spatial form of the labour process. From this standpoint, the thesis engages with labour process theory after Braverman (accusing it of often failing to link capitalist control to class processes) and with theories of class (which often ignore the social and spatial form of the labour process). In tying organising capacities of women workers at the enterprise level to changes in social and spatial form of the labour process, it is nevertheless argued that these capacities are also shaped at the national level by the legal framework for legitimate organising and by 'political space' in which the law in fact operates. In this regard, it is argued that, whilst the state often passes laws to protect labour standards, it does not grant workers the means to ensure such standards are actually enforced. The thesis also challenges the view that the recruitment of women is a strategy which employers deliberately use in the Philippine garments industry to limit industrial conflict. Against this assertion of a rational economic basis to women's employment, the thesis argues that women are employed for sewing jobs as a result of the sex-typing of such jobs; but that this is also more an effect than a cause as the feminisation of sewing in the modern garments industry is embedded in class processes in the nineteenth century in Europe and the United States. Gender is a dimension of labour control, but women workers in the garments industry are not employed to limit enterprise unionism

Bell Beaker people in Britain: migration, mobility and diet

The appearance of the distinctive ‘Beaker package’ marks an important horizon in British prehistory, but was it associated with immigrants to Britain or with indigenous converts? Analysis of the skeletal remains of 264 individuals from the British Chalcolithic–Early Bronze Age is revealing new information about the diet, migration and mobility of those buried with Beaker pottery and related material. Results indicate a considerable degree of mobility between childhood and death, but mostly within Britain rather than from Europe. Both migration and emulation appear to have had an important role in the adoption and spread of the Beaker package

UV Diagnostics of Galaxies from the Peak of Star-Formation to the Epoch of Reionization

The rest-frame UV emission from massive stars contains a wealth of information about the physical nature and conditions of star formation in galaxies. Using studies of the rest-frame UV, the past decade has witnessed the beginning of knowledge about the existence and properties of galaxies during the first few billion years after the Big Bang. This period of history corresponds to the formation of the first stars, the rapid formation of galaxy stellar populations, the reionization of the IGM, the production and dissemination of heavy elements, and the formation of the first black holes. Massive stars in these galaxies drive all of these events, and their light dominates the spectral energy distributions of galaxies. As we look to the 2020s, fundamental questions remain about the nature of these stellar populations and their evolution, from just before the peak of the cosmic star formation density (z~3), up to the epoch of reionization (z > 6). This next decade will provide transformative gains both in our ability to identify star-forming galaxies and accreting supermassive black holes at these early epochs with imaging surveys in the rest-frame UV (e.g., LSST, WFIRST). Ground-based, rest-frame UV spectroscopy on >20 m-class telescopes (e.g., GMT/TMT) offers the ability to investigate the astrophysical conditions in galaxies at the earliest cosmic times. This includes studies of the evolution in galaxy stellar populations, gas ionization (temperature, pressure), metallicity, and interstellar (and circumgalactic) gas kinematics and covering fractions. In this white paper, we describe the scientific prospects and the requirements for research in this area.Comment: White paper submitted to the Astro2020 Decadal Survey (8 papers, 4 figures

JWST's TEMPLATES for Star Formation: The First Resolved Gas-Phase Metallicity Maps of Dust-Obscured Star-Forming Galaxies at zz ∼\sim 4

We present the first spatially resolved maps of gas-phase metallicity for dust-obscured star-forming galaxies (DSFGs) at $z$ $\sim$ 4, from the JWST TEMPLATES Early Release Science program, derived from NIRSpec integral field unit spectroscopy of the H$\alpha$ and [NII] emission lines. Empirically derived literature optical line calibrations are used to determine that the sources are highly metal rich, with both appearing to display regions of supersolar metallicity, particularly in SPT2147-50. While we cannot rule out shocks or AGN in these regions, we suggest that the two systems have already undergone significant enrichment as a result of their extremely high star-formation rates. Utilising ALMA rest-frame 380$\mu$m continuum and [CI]($^3$P$_2$-$^3$P$_1$) line maps we compare metallicity and gas-to-dust ratio variations in the two galaxies, finding the two to be anticorrelated on highly resolved spatial scales, consistent with various literature studies of $z$ $\sim$ 0 galaxies. The data are indicative of the enormous potential of JWST to probe the enrichment of the interstellar medium on $\sim$kpc scales in extremely dust-obscured systems at $z$ $\sim$ 4 and beyond.Comment: 12 pages, 5 figures, submitted to Ap

JWST's TEMPLATES for Star Formation: The First Resolved Gas-phase Metallicity Maps of Dust-obscured Star-forming Galaxies at z ∼ 4

We present the first spatially resolved maps of gas-phase metallicity for two dust-obscured star-forming galaxies at z ∼ 4, from the JWST TEMPLATES Early Release Science program, derived from NIRSpec integral field unit spectroscopy of the Hα and [N ii] emission lines. Empirical optical line calibrations are used to determine that the sources are globally enriched to near-solar levels. While one source shows elevated [N ii]/Hα ratios and broad Hα emission consistent with the presence of an active galactic nucleus in a ≳1 kpc region, we argue that both systems have already undergone significant metal enrichment as a result of their extremely high star formation rates. Utilizing Atacama Large Millimeter/submillimeter Array rest-frame 380 μm continuum and [Ci](3P2–3P1) line maps we compare the spatial variation of the metallicity and gas-to-dust ratio in the two galaxies, finding the two properties to be anticorrelated on highly resolved spatial scales, consistent with various literature studies of z ∼ 0 galaxies. The data are indicative of the enormous potential of JWST to probe the enrichment of the interstellar medium on ∼kpc scales in extremely dust-obscured systems at z ∼ 4 and beyond

Effects of antiplatelet therapy on stroke risk by brain imaging features of intracerebral haemorrhage and cerebral small vessel diseases: subgroup analyses of the RESTART randomised, open-label trial

Background Findings from the RESTART trial suggest that starting antiplatelet therapy might reduce the risk of recurrent symptomatic intracerebral haemorrhage compared with avoiding antiplatelet therapy. Brain imaging features of intracerebral haemorrhage and cerebral small vessel diseases (such as cerebral microbleeds) are associated with greater risks of recurrent intracerebral haemorrhage. We did subgroup analyses of the RESTART trial to explore whether these brain imaging features modify the effects of antiplatelet therapy

Democratization and foreign policy in Southeast Asia: the case of the ASEAN Inter-Parliamentary Myanmar Caucus

This is an Author's Accepted Manuscript of an article published in Cambridge Review of International Affairs Vol. 22, Iss. 3, 2009 as published in the CAMBRIDGE REVIEW OF INTERNATIONAL AFFAIRS, 2009, copyright Taylor & Francis, available online at: http://www.tandfonline.com/10.1080/09557570903104008