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The Quasi-Coherent Oscillations of SS Cygni
Published online by Cambridge University Press: 12 April 2016
Abstract
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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