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Slingshot Prominences During Dwarf Nova Outbursts?

Published online by Cambridge University Press:  12 April 2016

D. Steeghs ,
K. Horne  and
T. R. Marsh
D. Steeghs
Affiliation:
Astronomical Institute, Utrecht University, The Netherlands
K. Horne
Affiliation:
Physics & Astronomy, University of St. Andrews, UK
T. R. Marsh
Affiliation:
Astronomy Group, University of Southampton, UK

Abstract

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We present phase-resolved spectroscopy of two dwarf novae, IP Peg and SS Cyg, observed in outburst with the WHT/ISIS spectropolarimeter. Doppler tomograms of several emission lines show peculiar narrow, stationary emission components.

Type
Non-Magnetic Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 71 - 72
Copyright
Copyright © Kluwer 1996

References

Horne, K., 1991, in “Fundamental Properties of CVs” ed. Shafter, A.W. (U. San Diego)Google Scholar