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Detection of the Irradiated Red Dwarf in WY Sge (Nova 1783)

Published online by Cambridge University Press:  12 April 2016

M. W. Somers ,
K. Mukai ,
T. Naylor  and
F.A. Ringwald
M. W. Somers
Affiliation:
Department of Physics, Keele University, ST5 5BG, UK
K. Mukai
Affiliation:
Office for Guest Investigator Programs, Code 668, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA
T. Naylor
Affiliation:
Department of Physics, Keele University, ST5 5BG, UK
F.A. Ringwald
Affiliation:
Department of Physics, Keele University, ST5 5BG, UK

Abstract

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We present infrared (IR) photometry and optical spectroscopy of the eclipsing old nova WY Sge. According to hibernation theorists the disc in a system a few centuries after outburst should be significantly fainter than in other, more recent, old novae but similar to the discs of dwarf novae in quiescence. Despite the apparent faintness of the late type star we have sufficient information to infer that the face closest to the white dwarf (WD) is irradiated.

Type
Novae & Symbiotic Stars
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 327 - 328
Copyright
Copyright © Kluwer 1996

References

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