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The Nova-Likes AC Cnc, RW Tri, UX UMa and the Nova DQ Her: Common and Different Properties

Published online by Cambridge University Press:  12 April 2016

E. S. Dmitrienko
E. S. Dmitrienko*
Affiliation:
Crimean Astrophysical Observatory, 334413, Crimea, Ukraine, e-mail:dmitrien@crao.crimea.ua

Abstract

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An analysis of the main photometric properties of the nova-like variables AC Cnc, RW Tri and UX UMa, and Nova Her 1934 (DQ Her) is presented. The analysis is based on simultaneous high-speed UBVRI photometry, covering several dozens of orbital cycles evenly distributed over 14 years (1982 ... 1995) for DQ Her, and over 11 years (1985 ... 1995) for the other three stars. All data have been obtained with the 1.25 m telescope at the Crimean Astrophysical Observatory.

Type
Non-Magnetic Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 13 - 14
Copyright
Copyright © Kluwer 1996

References

1. Dmitrienko, E.S., 1995, Astronomy Letters, 21, 171 Google Scholar