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The Algol-Type Binaries

  • Chapter
The Influence of Binaries on Stellar Population Studies

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 264))

Abstract

The nature of the circumstellar material in interacting binaries of the Algol-type, including the accretion disk, gas stream, high temperature plasma, and domains of outflow is reviewed. Mass transfer is compared in six similar systems with early B primaries and short-moderate periods that approximately represent a series of snapshots of such binaries during their slow evolutionary phase. Evidence for moderate systemic mass loss during the current and earlier stages is presented.

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Author information

Authors and Affiliations

  1. Space Sciences Center, University of Southern California, Los Angeles, CA, 90089-1341, USA

    Geraldine J. Peters

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  1. Geraldine J. Peters
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Editor information

Editors and Affiliations

  1. Astrophysical Institute, Vrije Universiteit Brussel, Belgium

    Dany Vanbeveren

  2. Technological Institute Group T, Leuven, Belgium

    Dany Vanbeveren

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© 2001 Springer Science+Business Media Dordrecht

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Peters, G.J. (2001). The Algol-Type Binaries. In: Vanbeveren, D. (eds) The Influence of Binaries on Stellar Population Studies. Astrophysics and Space Science Library, vol 264. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9723-4_6

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  • DOI: https://doi.org/10.1007/978-94-015-9723-4_6

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5745-7

  • Online ISBN: 978-94-015-9723-4

  • eBook Packages: Springer Book Archive

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