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The paper examines the need for sex fairness efforts for minority women (particularly black women), and relates those needs to the measurement of vocational interests. Much data is presented portraying the black woman as more likely to enter the labor force, more interested in doing so, more likely to work full time and continuously, and more necessary to the financial welfare of her family than her white counterpart. It is equally true that black women choose occupations traditional for women, are motivated perhaps more by a sense of responsibility than by achievement need, are much more traditional in their sex-role attitudes; thus, concern for the occupational options of white women can be no less directed towards them than towards any other women. An examination is presented of some of the technical aspects of the problem of preparing assessment instruments for minority group examinees in order to emphasize the need for further work in this area. The basic contention is that there may be a discontinuity or mis-match between the interest structures developed from the background of minority females and those possessed by the criterion groups used to validate an interest scale. (Author/AJ)

The Rossi X-ray Timing Explorer has observed the nearest radio galaxy, Centaurus A, in 13 intervals from 1996 August to 2009 February over the 3 - 200 keV band. Spectra accumulated over the 13 intervals were well described with an absorbed power law and an iron line. Cut-off power laws and Compton reflection from cold matter did not provide a better description. For the 2009 January observation we set a lower limit on the cutoff energy at over 2 MeV. The power spectral density function was generated from RXTE/ASM and PCA data as well as an XMM-Newton long look, and clear evidence for a break at 18(+18/-7) days (68% conf.) was seen. Given Cen A's high black hole mass and very low value of L(sub x)/L(sub Edd), the break was a factor of 17+/-9 times higher than the break frequency predicted by the McHardy and coworkers relation, which was empirically derived for a sample of objects, which are radio-quiet and accreting at relatively high values of L(sub bol)/L(sub Edd). We have interpreted our observations in the context of a clumpy molecular torus. The variability characteristics and the broadband spectral energy distribution, when compared to Seyferts, imply that the bright hard X-ray continuum emission may originate at the base of the jet, yet from behind the absorbing line of sight material, in contrast to what is commonly observed from blazars.