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The Possible Contribution from the Accretion Disk During the Quiescence of VW Hyi

Published online by Cambridge University Press:  12 April 2016

M. Huang ,
E. M. Sion ,
I. Hubeny ,
F. H. Cheng  and
P. Szkody
M. Huang
Affiliation:
Villanova University, Villanova, PA 19085, USA
E. M. Sion
Affiliation:
Villanova University, Villanova, PA 19085, USA
I. Hubeny
Affiliation:
Laboratory of Astronomy & Solar Physics, Code 681, NASA/GSFC, Greenbelt, MD 20771, USA
F. H. Cheng
Affiliation:
Dept. of Astrophysics, Univ. of Maryland, Collge Park, MD 20742, USA
P. Szkody
Affiliation:
Dept. of Astronomy, FM-20, Univ. of Washington, Seattle, WA 98195, USA

Abstract

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We have re-analyzed UV spectra of the dwarf nova VW Hyi during its quiescence, obtained with the Faint Object Spectrograph (FOS) on Hubble Space Telescope (HST), by considering the possible contribution from the accretion disk, which was not included in the previous analysis.

Type
Space Observations
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 247 - 248
Copyright
Copyright © Kluwer 1996

References

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