Building a blog cabin during a financial crisis: circuits of struggle in the digital enclosure

ManuscriptOne of the most pressing questions facing television studies is how to understand the migration of media production and consumption onto web applications which depend on user-generated content. Scholars inspired by the political economy of communication (PEC) tradition have focused on how the accumulation strategies of firms like Google enclose users in a web of commercial surveillance, thus facilitating the commodification of their online labor. However, this article argues that this focus on commercial enclosure has often led PEC scholars to overlook the political possibilities highlighted by autonomist Marxist theory?namely, that users, under certain conditions, can appropriate these networks and applications to contest relations of exploitation. This article offers a case analysis of Blog Cabin 2008, a DIY Network home improvement show, in order to explore this tension between the autonomy and enclosure of users. The findings of this case analysis suggest that producers indeed used the show?s blog to exploit fans? free labor. At the same time, fans also used the blog to constitute themselves as a community, to press demands on the show?s producers, and to explore connections between the class politics of the show and the wider political economy. A concluding section explores the theoretical and political significance of such unanticipated uses of the show?s blog

Australian attempt to internationalize accounting professional organizations

In 1928, the beginnings were laid for the International Accountants Corporation and Bookkeepers Institute of Australasia. This was followed in a few years by the International Institute of Accountants. This was an ambitious move to internationalize the professional accounting organizations of the world from Australia

Sexual Selection in Lekking Sage Grouse: Phenotypic Correlates of Male Mating Success

Mate choice cues in sage grouse were reinvestigated by analyzing relationships between male mating success and a range of suggested cues. Display cues were implicated by significant relationships between mating status (whether or not a male mated) and lek attendance, display rate (corrected for effects of female proximity and time of day) and an acoustic component related to temporal and frequency measures of a whistle emitted during the strut display. Although display rate and the acoustic component were intercorrelated, both exerted significant partial effects on mating success in multivariate analyses. These display measures also differed significantly between males. In contrast, mating success was not significantly related to measures of territory characteristics, including size and proximity to the lek center, or to body size. These results resolve discrepancies between previous studies and provide a basis for experimental analysis of the role of female choice in this lek system

The Evolution of Quasar CIV and SiIV Broad Absorption Lines Over Multi-Year Time Scales

We investigate the variability of CIV 1549A broad absorption line (BAL) troughs over rest-frame time scales of up to ~7 yr in 14 quasars at redshifts z>2.1. For 9 sources at sufficiently high redshift, we also compare CIV and SiIV 1400A absorption variation. We compare shorter- and longer-term variability using spectra from up to four different epochs per source and find complex patterns of variation in the sample overall. The scatter in the change of absorption equivalent width (EW), Delta EW, increases with the time between observations. BALs do not, in general, strengthen or weaken monotonically, and variation observed over shorter (<months) time scales is not predictive of multi-year variation. We find no evidence for asymmetry in the distribution of Delta EW that would indicate that BALs form and decay on different time scales, and we constrain the typical BAL lifetime to be >~30 yr. The BAL absorption for one source, LBQS 0022+0150, has weakened and may now be classified as a mini-BAL. Another source, 1235+1453, shows evidence of variable, blue continuum emission that is relatively unabsorbed by the BAL outflow. CIV and SiIV BAL shape changes are related in at least some sources. Given their high velocities, BAL outflows apparently traverse large spatial regions and may interact with parsec-scale structures such as an obscuring torus. Assuming BAL outflows are launched from a rotating accretion disk, notable azimuthal symmetry is required in the outflow to explain the relatively small changes observed in velocity structure over times up to 7 yr

The X-Ray Properties of the Optically Brightest Mini-BAL Quasars from the Sloan Digital Sky Survey

We have compiled a sample of 14 of the optically brightest radio-quiet quasars ($m_{i}$~$\le$~17.5 and $z$~$\ge$~1.9) in the Sloan Digital Sky Survey Data Release 5 quasar catalog that have C IV mini-BALs present in their spectra. X-ray data for 12 of the objects were obtained via a Chandra snapshot survey using ACIS-S, while data for the other two quasars were obtained from archival XMM-Newton observations. Joint X-ray spectral analysis shows the mini-BAL quasars have a similar average power-law photon index ($\Gamma\approx1.9$) and level of intrinsic absorption ($N_H \lesssim 8\times 10^{21} \ {\rm cm}^{-2}$) as non-BMB (neither BAL nor mini-BAL) quasars. Mini-BAL quasars are more similar to non-BMB quasars than to BAL quasars in their distribution of relative X-ray brightness (assessed with $\Delta\alpha_{\rm ox}$). Relative colors indicate mild dust reddening in the optical spectra of mini-BAL quasars. Significant correlations between $\Delta\alpha_{\rm ox}$ and UV absorption properties are confirmed for a sample of 56 sources combining mini-BAL and BAL quasars with high signal-to-noise ratio rest-frame UV spectra, which generally supports models in which X-ray absorption is important in enabling driving of the UV absorption-line wind. We also propose alternative parametrizations of the UV absorption properties of mini-BAL and BAL quasars, which may better describe the broad absorption troughs in some respects.Comment: ApJ accepted; 21 pages, 11 figures, and 9 table

The Rates of Combination of the Isolated Chains of Human Hemoglobin with Oxygen

Abstract The rates of combination of the isolated chains of human hemoglobin with oxygen have been measured by flash photolysis and stopped flow methods. The two experimental methods give similar results, and furthermore the data compare well with those obtained recently by the temperature jump relaxation method. The measured association rates are compared with the values predicted from the previously measured equilibrium and dissociation rate constants. A significant discrepancy is noted in the case of the β chains. In addition, the rates of replacement of oxygen by carbon monoxide as functions of the relative ligand concentrations have been measured, and the observed dependences are compared to those predicted from the equilibrium and kinetic constants for the individual liganding reactions