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Non-Magnetic Cataclysmic Variables in the ROSAT WFC Survey

Published online by Cambridge University Press:  12 April 2016

Peter J. Wheatley
Peter J. Wheatley*
Affiliation:
Astronomical Institute, Utrecht University, Postbus 80 000, 3508 TA Utrecht, NL

Abstract

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Six non-magnetic cataclysmic variables were detected during the ROSAT WFC survey; four dwarf novae and two nova-like variables. In two dwarf novae (VW Hyi & SS Cyg) the flux evolution through outburst was followed across a broad wavelength range. The two other detections (Z Cam & RX J0640−24) also suggest the presence of distinct luminous EUV emission components; supporting the view that such components are a ubiquitous feature of dwarf nova outbursts. Two bright nova-like variables were detected, but these detections are found to be consistent with the soft tail of the X-ray emission.

Type
VI. Cataclysmic Variable Stars
Information
International Astronomical Union Colloquium , Volume 152: Astrophysics in the Extreme Ultraviolet , 1996 , pp. 337 - 341
Copyright
Copyright © Kluwer 1996

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