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Polarization from Be Disks with 1-Armed Density Waves

Published online by Cambridge University Press:  12 April 2016

R. Ignace
R. Ignace*
Affiliation:
Physics and Astronomy, University of Glasgow, Scotland, UK

Abstract

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The polarization of Be disks that are not axisymmetric is discussed, with results given for one-armed density waves or global disk oscillations (GDO). Polarimetric diagnostics of electron scattering Be disks are presented, including the expected behavior at (a) optical wavelengths where the star is the dominant source of luminosity and (b) infrared wavelengths where the disk is more luminous than the star. Results for detached disks are given. A qualitative discussion of polarization at Hα is also presented.

Information

Type
6. Disks
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000, pp. 452 - 459
Copyright
Copyright © Astronomical Society of the Pacific 2000

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