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The Quasi-Coherent Oscillations of SS Cygni

Published online by Cambridge University Press:  12 April 2016

Christopher W. Mauche
Christopher W. Mauche*
Affiliation:
Lawrence Livermore National Laboratory, L–41, P.O. Box 808, Livermore, CA 94550

Abstract

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Properties of the quasi-coherent oscillations in the extreme ultraviolet flux of the dwarf nova SS Cygni are described.

Type
Part 6. Disk-Star-Magnetosphere Interaction
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 251 - 255
Copyright
Copyright © Astronomical Society of the Pacific 1997

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