19,329 research outputs found

    Jewish Studies: Are They Ethnic?

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    The history of Jewish studies has not yet been written. Scholars engaged in this field, however, are beginning to subject it to searching analysis. Pertinent articles have appeared that offer two extreme positions on the development of Jewish studies: one sees the increase in Jewish studies as the result of heightened Jewish self-awareness during the late 1960s because of the Six Day War, growing interest in the Holocaust, and the influence of rising black and ethnic consciousnesses that resulted in the establishment of academic programs. The other, usually a reaction to the first view, argues that the study of Hebraica and Judaica has held an ancient and honorable place in the traditional university curriculum

    The Spaces Between Numbers: Getting International Data on Higher Education Straight

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    Argues that the participation and attainment data used in international comparisons do not reflect the performance objectives of higher education systems. Suggests economic and demographic frameworks for interpreting data and changes in data collection

    Learning Accountability From Bologna: A Higher Education Policy Primer

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    Outlines issues from the European Higher Education Area's Bologna Process, a framework for standardizing degree qualifications, credits and curriculum reform, and supplementary documentation. Suggests changes to raise accountability in U.S. institutions

    Stellar model atmospheres with magnetic line blanketing. III. The role of magnetic field inclination

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    Context. See abstract in the paper. Aims. In the last paper of this series we study the effects of the magnetic field, varying its strength and orientation, on the model atmosphere structure, the energy distribution, photometric colors and the hydrogen Balmer line profiles. We compare with the previous results for an isotropic case in order to understand whether there is a clear relation between the value of the magnetic field angle and model changes, and to study how important the additional orientational information is. Also, we examine the probable explanation of the visual flux depressions of the magnetic chemically peculiar stars in the context of this work. Methods. We calculated one more grid of the model atmospheres of magnetic A and B stars for different effective temperatures (Teff=8000K, 11000K, 15000K), magnetic field strengths (B=0, 5, 10, 40 kG) and various angles of the magnetic field (Omega=0-90 degr) with respect to the atmosphere plane. We used the LLmodels code which implements a direct method for line opacity calculation, anomalous Zeeman splitting of spectral lines, and polarized radiation transfer. Results. We have not found significant changes in model atmosphere structure, photometric and spectroscopic observables or profiles of hydrogen Balmer lines as we vary the magnetic field inclination angle Omega. The strength of the magnetic field plays the main role in magnetic line blanketing. We show that the magnetic field has a clear relation to the visual flux depressions of the magnetic CP stars. Conclusions. See abstract in the paper.Comment: 10 pages, 5 figure
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