Mediated intimacy and postfeminism: A discourse analytic examination of sex and relationships advice in a women's magazine

This paper uses a discourse analytic perspective to analyse sex and relationship advice in a best-selling women's magazine. It identifies three different interpretative repertoires which together structure constructions of sexual relationships: the intimate entrepreneurship repertoire, organised around plans, goals and the scientific management of relationships; men-ology, in which women are instructed in how to learn to please men; and transforming the self, which calls on women to remodel their interior lives in order to construct a desirable subjectivity. The paper considers each repertoire in turn, and also looks at how they work together in order to privilege men and heterosexuality. Discussion focuses in particular on the postfeminist nature of the advice, in which pre-feminist, feminist and anti-feminist ideas are entangled in such a way as to make gender ideologies more pernicious and difficult to contest

Search for Gravitational Wave Bursts from Six Magnetars

Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitation of non-radial modes which would emit gravitational waves (GWs). We present the results of a search for GW bursts from six galactic magnetars that is sensitive to neutron star f-modes, thought to be the most efficient GW emitting oscillatory modes in compact stars. One of them, SGR 0501+4516, is likely similar to 1 kpc from Earth, an order of magnitude closer than magnetars targeted in previous GW searches. A second, AXP 1E 1547.0-5408, gave a burst with an estimated isotropic energy >10(44) erg which is comparable to the giant flares. We find no evidence of GWs associated with a sample of 1279 electromagnetic triggers from six magnetars occurring between 2006 November and 2009 June, in GW data from the LIGO, Virgo, and GEO600 detectors. Our lowest model-dependent GW emission energy upper limits for band-and time-limited white noise bursts in the detector sensitive band, and for f-mode ringdowns (at 1090 Hz), are 3.0 x 10(44)d(1)(2) erg and 1.4 x 10(47)d(1)(2) erg, respectively, where d(1) = d(0501)/1 kpc and d(0501) is the distance to SGR 0501+4516. These limits on GW emission from f-modes are an order of magnitude lower than any previous, and approach the range of electromagnetic energies seen in SGR giant flares for the first time.United States National Science FoundationScience and Technology Facilities Council of the United KingdomMax-Planck-SocietyState of Niedersachsen/GermanyItalian Istituto Nazionale di Fisica NucleareFrench Centre National de la Recherche ScientifiqueAustralian Research CouncilCouncil of Scientific and Industrial Research of IndiaIstituto Nazionale di Fisica Nucleare of ItalySpanish Ministerio de Educacion y CienciaConselleria d'Economia Hisenda i Innovacio of the Govern de les Illes BalearsFoundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific ResearchPolish Ministry of Science and Higher EducationFoundation for Polish ScienceRoyal SocietyScottish Funding CouncilScottish Universities Physics AllianceNational Aeronautics and Space Administration NNH07ZDA001-GLASTCarnegie TrustLeverhulme TrustDavid and Lucile Packard FoundationResearch CorporationAlfred P. Sloan FoundationRussian Space AgencyRFBR 09-02-00166aIPN JPL Y503559 (Odyssey), NASA NNG06GH00G, NASA NNX07AM42G, NASA NNX08AC89G (INTEGRAL), NASA NNG06GI896, NASA NNX07AJ65G, NASA NNX08AN23G (Swift), NASA NNX07AR71G (MESSENGER), NASA NNX06AI36G, NASA NNX08AB84G, NASA NNX08AZ85G (Suzaku), NASA NNX09AU03G (Fermi)Astronom

It's a different world: a dialog on the attention-based view in a post-Chandlerian world

In this Dialog, seven scholars consider the theoretical implications and research opportunities a changing environment presents for the Attention-Based View (ABV). With its roots in the 1950s Carnegie School, ABV is expanding and evolving in ways that accommodate the changes in the corporate context characterized by distributed, porous structures of organizational networks such as ecosystems and platforms. The authors emphasize a shift toward a more dynamic orientation of this research, one that addresses the challenges of sustaining coherent attention and sensemaking, a shift from quantity to quality of attention, and how corporate communications ranging from formalized strategy presentations to less formal social media communications can spin attention in ways that lead to intended as well as unintended outcomes. Emerging organizational trends open up radically different perspectives on attention: today's superstar firms draw new kinds of attention and many new business models are based upon the attraction and selling of customer attention

Video Conferencing Guidelines for Faculty and Students in Graduate Online Courses (Doctoral dissertation

Abstract A review of the literature revealed that established guidelines were not available to assist faculty who use video conferencing in their online graduate courses. In an effort to address this need, a self-evaluation study was completed with faculty who teach such courses. Drawing on the results of this study together with published Netiquette guidelines and a survey of other extant literature, a set of Video Conferencing Guidelines was created

Differential Scanning Calorimetry and Evolved Gas Analysis at Mars Ambient Conditions Using the Thermal Evolved Gas Analyzer (TEGA)

Differential Scanning Calorimetry (DSC) combined with evolved gas analysis (EGA) is a well developed technique for the analysis of a wide variety of sample types with broad application in material and soil sciences. However, the use of the technique for samples under conditions of pressure and temperature as found on other planets is one of current C development and cutting edge research. The Thermal Evolved Gas Analyzer (MGA), which was designed, built and tested at the University of Arizona's Lunar and Planetary Lab (LPL), utilizes DSC/EGA. TEGA, which was sent to Mars on the ill-fated Mars Polar Lander, was to be the first application of DSC/EGA on the surface of Mars as well as the first direct measurement of the volatile-bearing mineralogy in martian soil