What can we learn from ζ Aur binary systems?

Schröder, K.-P.

doi:10.1007/978-94-009-2969-2_73

What can we learn from ζ Aur binary systems?

K.-P. Schröder⁵

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 145))

Abstract

ζ Aur binaries are wide eclipsing systems (P≃1...10 yrs), containing a late supergiant primary (G to M type) and an early dwarf companion (AO V ... B3 V). Some recent studies of wind phenomena (mass loss rates), chromospheric properties and wind acceleration (of the supergiant) as well as wind accretion phenomena introduced by the gravitational interaction with the companion are presented, summarizing previous work of the Hamburg ‘binary wind team’(mainly D. Reimers, R. Baade, A. Che-Bohnenstengel, K. Hempe, K.-P. Schröder).

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Authors and Affiliations

Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 2050, Hamburg 80, West Germany
K.-P. Schröder

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K.-P. Schröder
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Editors and Affiliations

Institute of Astronomy, Nicolaus Copernicus University, Torun, Poland
Joanna Mikolajewska
Institut d’Astrophysique, CNRS, Paris, France
Michael Friedjung
Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts, USA
Scott J. Kenyon
Istituto Astrofisica Spaziale, CNR, Frascati, Italy
Roberto Viotti

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Schröder, KP. (1988). What can we learn from ζ Aur binary systems?. In: Mikolajewska, J., Friedjung, M., Kenyon, S.J., Viotti, R. (eds) The Symbiotic Phenomenon. Astrophysics and Space Science Library, vol 145. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2969-2_73

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DOI: https://doi.org/10.1007/978-94-009-2969-2_73
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7833-7
Online ISBN: 978-94-009-2969-2
eBook Packages: Springer Book Archive

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