OSHA Enforcement, Industrial Compliance and Workplace Injuries

This paper develops and tests a three-equation simultaneous model of OSHA enforcement behavior, industrial compliance and workplace injuries. The enforcement equation is based on the assumption that OSHA acts as a political institution that gains support through the transfer of wealth from firms to employees; the empirical results are largely consistent with this notion. Contrary to previous work, we find that OSHA enforcement efforts have, indeed, had a statistically significant impact on industrial compliance and, further, that this compliance has led to a statistically significant decrease in worker injuries. The point estimate of the elasticity of the lost workday rate with respect to the OSHA inspection rate is -.04.

Predation through Regulation: The Wage and Profit Impacts of OSHA and EPA

This paper documents the importance of studying the indirect effects of OSHA and EPA regulations -- the competitive advantages which arise from the asymmetrical distributions of regulatory impact among different types of firms. We argue that if the competitive advantage gained through indirect effects is sufficiently large, it can more than offset any direct costs producing a net benefit for the regulated firm and its workers. The indirect effects of OSHA and EPA regulations arise in two ways. The first source is compliance asymmetries, whereby one firm suffers a greater cost burden even when regulations are evenly enforced across firms. The second source is enforcement asymmetry, whereby regulations are more vigorously enforced against certain firms. Earlier research shows that these asymmetries do exist and are based on firm size, unionization, and regional location. In this paper we empirically document that the indirect effects produced by these asymmetries mitigate the direct costs of regulations for manyfirms. Large, unionized firms in the Frostbelt are clearly gaining wealth at the expense of small, nonunionized firms in the Sunbelt.

QSO environments at intermediate redshifts

We have made a survey of quasar environments at 0.5 < z < 0.8, using a sample of both radio-loud and radio-quiet quasars matched in B-band luminosity. Our observations include images of background control fields to provide a good determination of the field galaxy counts. About 10 per cent of the quasars appear to live in rich clusters, whereas approximately 45 per cent live in environments similar to that of field galaxies. The richness of galaxies within a 0.5 Mpc radius around the radio-quiet quasars is found to be indistinguishable from the richness around the radio-loud quasars, corresponding on average to groups or poorer clusters of galaxies. Comparing the galaxy richness in the radio-loud quasar fields with quasar fields in the literature, we find no evidence of an evolution in the environment with epoch. Instead, a weak, but significant correlation between quasar radio luminosity and environmental richness is present. It is thus possible that the environments of quasars, at least the powerful ones, do not evolve much between the present epoch and z \approx 0.8.Comment: 6 pages, 4 figures, to appear in the proc. of the workshop `QSO hosts and their environments', IAA, Granada 10-12 Jan, 200

The Abundances Of Polyacetylenes Toward CRL618

We present a mid-infrared high spectral resolution spectrum of CRL618 in the frequency ranges 778-784 and 1227-1249 cm(-1) (8.01-8.15 and 12.75-12.85 mu m) taken with the Texas Echelon-cross-Echelle Spectrograph (TEXES) and the Infrared Telescope Facility (IRTF). We have identified more than 170 rovibrational lines arising from C2H2, HCN, C4H2, and C6H2. We have found no unmistakable trace of C8H2. The line profiles display a complex structure suggesting the presence of polyacetylenes in several components of the circumstellar envelope (CSE). We derive total column densities of 2.5x10(17), 3.1x10(17), 2.1x10(17), 9.3x10(16) cm(-2), and less than or similar to 5x10(16) cm(-2) for HCN, C2H2, C4H2, C6H2, and C8H2, respectively. The observations indicate that both the rotational and vibrational temperatures in the innermost CSE depend on the molecule, varying from 100 to 350 K for the rotational temperatures and 100 to 500 K for the vibrational temperatures. Our results support a chemistry in the innermost CSE based on radical-neutral reactions triggered by the intense UV radiation field.Spanish Ministerio de Educacion y Ciencia ESP2004-665, AYA2003-2785"Comunidad de Madrid" government S-0505/ESP-0237European Community MCRTN-CT-2004-51230CSICCONACyT SEP-2004-C01-47090UNAMNSF AST-0708074Astronom