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The Nature of RW Sextantis

Published online by Cambridge University Press:  12 April 2016

U. Bolick ,
K. Beuermann ,
A. Bruch  and
R. Lenzen
U. Bolick
Affiliation:
Institut für Astronomie und Astrophysik, TU Berlin, F.R.G.
K. Beuermann
Affiliation:
Institut für Astronomie und Astrophysik, TU Berlin, F.R.G. Max-Planck-Institut für Extraterrestrische Physik, Garching, F.R.G.
A. Bruch
Affiliation:
Astronomisches Institut, Universität Münster, F.R.G.
R. Lenzen
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg, F.R.G.

Abstract

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Photometry and first results of extensive CCD-spectroscopy of the UX UMa system RW Sex are presented. The period is found to be P = 0.24486 days and the semi-amplitude of the radial velocity is K1 = 101 km s−1. The mass of a Roche-lobe filling secondary is M2 = (0.54±0.09) Mo and, for M1 ≧ M2, the mass ratio is M1/M2 = 1.5±0.5. The accretion rate is about (2–3) 1017 g/s. The model for RW Sex by Greenstein and Oke is discussed and rejected.

Type
II. Radio, IR and Optical Observations
Information
International Astronomical Union Colloquium , Volume 93: Cataclysmic Variables: Recent Multi-Frequency Observations and Theoretical Developments , 1987 , pp. 175 - 179
Copyright
Copyright © Reidel 1987

References

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