Women's Rights, Human Rights, and Duties: From Domination to Partnership

The idea of women's rights as human rights can facilitate our identifying the causes, consequences, and potential remedies for the current quagmire in which we find themselves, but it needs some reformulation. To the traditional understandings of human rights, I add four conceptual tools: (1) Mahatma Gandhi’s idea of the counterparts of rights and duties, (2) Eisler’s concept of partnership (as opposed to dominator) societies, (3) Johan Galtung’s expansion of our conception of violence to include its structural and cultural forms, and, finally, (4) the literature on nonviolence as a path to mobilization and transformation that resists existing social structures and builds new ones

A Glimpse of Goffman

Dr. Lester R. Kurtz, Professor of George Mason University, wrote this memoir at the request of Dmitri Shalin and gave his permission to post the present version in the Erving Goffman Archives

Spectrophotometric Distances to Galactic H\,{\sc{ii}} Regions

We present a near infrared study of the stellar content of 35 H\,{\sc{ii}} regions in the Galactic plane. In this work, we have used the near infrared domain $J-$, $H-$ and $K_{s}-$ band color images to visually inspect the sample. Also, color-color and color-magnitude diagrams were used to indicate ionizing star candidates, as well as, the presence of young stellar objects such as classical TTauri Stars (CTTS) and massive young stellar objects (MYSOs). We have obtained {\it Spitzer} IRAC images for each region to help further characterize them. {\it Spitzer} and near infrared morphology to place each cluster in an evolutionary phase of development. {\it Spitzer} photometry was also used to classify the MYSOs. Comparison of the main sequence in color-magnitude diagrams to each observed cluster was used to infer whether or not the cluster kinematic distance is consistent with brightnesses of the stellar sources. We find qualitative agreement for a dozen of the regions, but about half the regions have near infrared photometry that suggests they may be closer than the kinematic distance. A significant fraction of these already have spectrophotometric parallaxes which support smaller distances. These discrepancies between kinematic and spectrophotometric distances are not due to the spectrophotometric methodologies, since independent non-kinematic measurements are in agreement with the spectrophotometric results. For instance, trigonometric parallaxes of star-forming regions were collected from the literature and show the same effect of smaller distances when compared to the kinematic results. In our sample of H\,{\sc{ii}} regions, most of the clusters are evident in the near infrared images. Finally, it is possible to distinguish among qualitative evolutionary stages for these objects.Comment: 59 pages, 146 figures and 4 tables. MNRAS accepte

Resolved 24.5 micron emission from massive young stellar objects

Massive young stellar objects (MYSO) are surrounded by massive dusty envelopes. Our aim is to establish their density structure on scales of ~1000 AU, i.e. a factor 10 increase in angular resolution compared to similar studies performed in the (sub)mm. We have obtained diffraction-limited (0.6") 24.5 micron images of 14 well-known massive star formation regions with Subaru/COMICS. The images reveal the presence of discrete MYSO sources which are resolved on arcsecond scales. For many sources, radiative transfer models are capable of satisfactorily reproducing the observations. They are described by density powerlaw distributions (n(r) ~ r^(-p)) with p = 1.0 +/-0.25. Such distributions are shallower than those found on larger scales probed with single-dish (sub)mm studies. Other sources have density laws that are shallower/steeper than p = 1.0 and there is evidence that these MYSOs are viewed near edge-on or near face-on, respectively. The images also reveal a diffuse component tracing somewhat larger scale structures, particularly visible in the regions S140, AFGL 2136, IRAS 20126+4104, Mon R2, and Cep A. We thus find a flattening of the MYSO envelope density law going from ~10 000 AU down to scales of ~1000 AU. We propose that this may be evidence of rotational support of the envelope (abridged).Comment: 21 pages, accepted for A&

Globalisation, the practice of devotional songs and poems and the linguistic repertoires of young British Muslims

This article provides empirical data from transnational religious contexts which highlight the complexity, fluidity and indexicality of language and religious practices in globalising settings. Through an examination of the role of devotional song and poetry in the Islamic world, and in particular, among young multilingual and multivarietal British Muslims, an attempt is made to show how globalising processes of the present age contribute to, on the one hand, novel forms of language resources and innovative religious practices and, on the other, co-existing traditional approaches to faith and language practices. It also shows how young people deploy their linguistic repertoires and language resources in order to re-construct their religious and linguistic identities. A conclusion is presented that such practices, whilst drawing on old and traditional roots, become transformed when enacted in these newer settings, both linguistically and religiously