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The β Lyrae Puzzle

Published online by Cambridge University Press:  12 April 2016

A.P. Linnell
A.P. Linnell*
Affiliation:
Astronomy Department, University of Washington, Seattle, WA 98195, USA

Abstract

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Accurate simulation of optical wavelength CCD spectra is possible by adopting a black-body representation for the radiation characteristics of the β Lyrae accretion disk rim. Application of this model to IUE spectra shows that the anomalous system light curves, in the satellite UV, arise from a source of radiation, not included in the current model, which is visible during the phase 0.0 eclipse.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 187: Exotic Stars as Challenges to Evolution , 2002 , pp. 209 - 214
Copyright
Copyright © Astronomical Society of the Pacific 2002

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