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Preliminary analysis of a Hubble FOS spectrum of VW Hyi in quiescence: A DAZQ white dwarf and accretion belt/ring

Published online by Cambridge University Press:  12 April 2016

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

Abstract

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We present a preliminary analysis of the UV spectrum of the dwarf nova VW Hyi during early quiescence, obtained with the Faint Object Spectrograph (FOS) on the Hubble Space Telescope (HST). The data were obtained approximately one day after the end of a normal outburst.

Type
Space Observations
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 249 - 250
Copyright
Copyright © Kluwer 1996

References

Huang, M., Sion, E.M., Hubeny, I., et al., 1996, these proceedings, p247 CrossRefGoogle Scholar
Sion, E.M., Szkody, P., Cheng, F.H., Huang, M., 1995, Ap. J., 444, L97 Google Scholar