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The β Lyrae Puzzle
Published online by Cambridge University Press: 12 April 2016
Abstract
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