TOWARD UNDERSTANDING THE B[e] PHENOMENON. IV. MODELING OF IRAS 00470+6429
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/721/i=2/a=1079/pdf
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1. Non‐LTE Monte Carlo Radiative Transfer. I. The Thermal Properties of Keplerian Disks around Classical Be Stars
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4. On the Determination of the Rotational Oblateness of Achernar
5. Achernar: Rapid Polarization Variability as Evidence of Photospheric and Circumstellar Activity
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