Explore the vast range of titles available.

Sexual harassment in the workplace has emerged in the past two decades as one of the most complex and emotional issues facing employers, employees, and human resource professionals today. In 1980, the Equal Employment Opportunity Commission (EEOC) declared sexual harassment a violation of Title VII of the Civil Rights Act of 1964. Sexual harassment is unwelcome behavior of a sexual nature that makes someone feel uncomfortable or unwelcome in the workplace by focusing attention on their gender instead of on their professional qualifications. A look at the past shows that, despite its explosion into the national consciousness with the Clarence Thomas confirmation hearings, sexual harassment evolved as a workplace issue over the past quarter-century. An employer's obligations with regard to sexual harassment arise before any act of sexual harassment occurs. The EEOC requires all organizations with more than 15 employees to develop a sexual harassment policy, to make that policy public, and train employees in issues of sexual harassment.

Cites sexual harassment as one of the most complex and emotional issues facing the business community. Briefly defines sexual harassment and the circumstances in which it can occur. Looks at the evolution of sexual harassment politics and discusses some landmark case law. Outlines the obligations of employers and provides the guidelines of the Equal Employment Opportunity Commission. Suggests that the best way to avoid potential litigation is to take the issue seriously.

The umbrella cells that line the bladder are mechanosensitive, and bladder filling increases the apical surface area of these cells; however, the upstream signals that regulate this process are unknown. Increased pressure stimulated ATP release from the isolated uroepithelium of rabbit bladders, which was blocked by inhibitors of vesicular transport, connexin hemichannels, ABC protein family members, and nucleoside transporters. Pressure-induced increases in membrane capacitance (a measure of apical plasma membrane surface area where 1 microF approximately equals 1 cm2) were inhibited by the serosal, but not mucosal, addition of apyrase or the purinergic receptor antagonist PPADS. Upon addition of purinergic receptor agonists, increased capacitance was observed even in the absence of pressure. Moreover, knockout mice lacking expression of P2X2 and/or P2X3 receptors failed to show increases in apical surface area when exposed to hydrostatic pressure. Treatments that prevented release of Ca2+ from intracellular stores or activation of PKA blocked ATPgammaS-stimulated changes in capacitance. These results indicate that increased hydrostatic pressure stimulates release of ATP from the uroepithelium and that upon binding to P2X and possibly P2Y receptors on the umbrella cell, downstream Ca2+ and PKA second messenger cascades may act to stimulate membrane insertion at the apical pole of these cells.

ABSTRACT In our effort to complete the census of low-mass stars and brown dwarfs in the immediate solar neighborhood, we present spectra, photometry, proper motions, and distance estimates for 42 low-mass star and brown dwarf candidates discovered by the Wide-field Infrared Survey Explorer (WISE). We also present additional follow-up information on 12 candidates selected using WISE data but previously published elsewhere. The new discoveries include 15 M dwarfs, 17 L dwarfs, five T dwarfs, and five objects of other types. Among these discoveries is a newly identified \"unusually red L dwarf\" (WISE J223527.07 + 451140.9), four peculiar L dwarfs whose spectra are most readily explained as unresolved L + T binary systems, and a T9 dwarf (WISE J124309.61 + 844547.8). We also show that the recently discovered red L dwarf WISEP J004701.06 + 680352.1 may be a low-gravity object and hence young and potentially low-mass (< 25 MJup).

In our effort to complete the census of low-mass stars and brown dwarfs in the immediate solar neighborhood, we present spectra, photometry, proper motions, and distance estimates for 42 low-mass star and brown dwarf candidates discovered by the Wide-field Infrared Survey Explorer (WISE). We also present additional follow-up information on 12 candidates selected usingWISEdata but previously published elsewhere. The new discoveries include 15 M dwarfs, 17 L dwarfs, five T dwarfs, and five objects of other types. Among these discoveries is a newly identified “unusually red L dwarf” (WISE J223527.07 + 451140.9 J 223527.07 + 451140.9 ), four peculiar L dwarfs whose spectra are most readily explained as unresolvedL + T L + T binary systems, and a T9 dwarf (WISE J124309.61 + 844547.8 J 124309.61 + 844547.8 ). We also show that the recently discovered red L dwarfWISEP J004701.06 + 680352.1 J 004701.06 + 680352.1 may be a low-gravity object and hence young and potentially low-mass (< 25 M Jup < 25     M Jup ).

In our effort to complete the census of low-mass stars and brown dwarfs in the immediate Solar Neighborhood, we present spectra, photometry, proper motions, and distance estimates for forty-two low-mass star and brown dwarf candidates discovered by the Wide-field Infrared Survey Explorer (WISE). We also present additional follow-up information on twelve candidates selected using WISE data but previously published elsewhere. The new discoveries include fifteen M dwarfs, seventeen L dwarfs, five T dwarfs, and five objects of other type. Among these discoveries is a newly identified \"unusually red L dwarf\" (WISE J223527.07+451140.9), four peculiar L dwarfs whose spectra are most readily explained as unresolved L+T binary systems, and a T9 dwarf (WISE J124309.61+844547.8). We also show that the recently discovered red L dwarf WISEP J004701.06+680352.1 (Gizis et al. 2012) may be a low-gravity object and hence young and potentially low mass (< 25 MJup).