Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-30T05:39:55.792Z Has data issue: false hasContentIssue false

Cataclysmic Variables: A ’SWOT’ Analysis

Published online by Cambridge University Press:  12 April 2016

Brian Warner*
Affiliation:
Department of Astronomy, University of Cape Town, Rondebosch 7700, South Africa

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A brief review of the nature and subtypes of cataclysmic variables (CVs) is given. The catalogue of CVs is still very incomplete. All-sky surveys should add large numbers of CVs, which will improve knowledge of the space density of these systems. It is pointed out that the nova-like variables, which are the most difficult to discover, are the subtype having the highest space density. Their discovery is therefore the highest priority – they fix the frequency of CVs, which is important in population syntheses of binary stars.

Type
V. Variability Study
Copyright
Copyright © Astronomical Society of the Pacific 2001

References

Allen, C.W. 1954, MNRAS, 114, 387 CrossRefGoogle Scholar
Beuermann, K. & Burwitz, V. 1995, ASP Conf.Ser. 85, 99 Google Scholar
Debehogne, H. 1990, IAU Circ.No. 5131Google Scholar
Downes, R, Webbink, R.F. & Shara, M.M. 1997, PASP, 109, 345 CrossRefGoogle Scholar
Duerbeck, H.W. 1990, IAU Colloq.No. 122, p. 134 CrossRefGoogle Scholar
Liu, W. & Hu, J.Y. 2000, ApJS, 128, 387 CrossRefGoogle Scholar
Liu, W., Hu, J.Y., Li, Z.Y. & Cao, L. 1999, ApJS, 122, 257 CrossRefGoogle Scholar
Patterson, J. 1984, ApJS, 54, 443 CrossRefGoogle Scholar
Patterson, J. 1998, PASP, 110, 1132 CrossRefGoogle Scholar
Warner, B. 1974, MNASSA, 33, 21 Google Scholar
Warner, B. 1987, MNRAS, 227, 23 CrossRefGoogle Scholar
Warner, B. 1995, Cataclysmic Variable Stars, Cambridge University Press CrossRefGoogle Scholar
Warner, B. 2000, PASP, 112, 1523 CrossRefGoogle Scholar