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Humps and Superhumps

Published online by Cambridge University Press:  12 April 2016

G.T. Bath ,
A.C. Edwards  and
V.J. Mantle
G.T. Bath
Affiliation:
Department of Astrophysics, Oxford
A.C. Edwards
Affiliation:
Department of Astrophysics, Oxford
V.J. Mantle
Affiliation:
Department of Astrophysics, Oxford

Extract

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It is now well established, following the classic work of Smak, Warner and Nather, that discs in dwarf novae possess an anisotropic radiation pattern responsible for the hump, or shoulder, that occurs prior to eclipse in the quiescent state, and, in systems with suitable inclination such as TT Gem, responsible also for the primary eclipse itself. In systems with higher inclination such as Z Cha, the primary eclipse is composed of both this anisotropic disc component and the inner-disc/white-dwarf primary component.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 72: Cataclysmic Variables and Related Objects , 1983 , pp. 69 - 76
Copyright
Copyright © Reidel 1983

References

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