Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-23T15:33:15.674Z Has data issue: false hasContentIssue false
  • English
  • Français

Cataclysmic Variables in a White Dwarf Survey at the South Galactic Pole

Published online by Cambridge University Press:  12 April 2016

I. Bues
I. Bues*
Affiliation:
Dr. Remeis-Sterwarte Bamberg, Astronomical Institute, University Erlangen-Nürnberg, Bamberg, F.R.G.

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.

During a ¡photometric and spectrophotometric survey of 200 white dwarf candidates with in a field around the South Galactic Pole two new cataclysmic variables have been identified and new observations of one already known object have been accumulated. Observations in the visible and UV-region show variability and differences in spectral type. If compared to the numbers of cataclysmic variables/white dwarfs as computed by Ritter and Burkert (1985)there is a shortage of a factor of 5.

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. 75 - 79
Copyright
Copyright © Reidel 1987

References

Bues, I., 1985, Proc. ESA-Workshop, ESA SP-236, 215 Google Scholar
Green, R.F., Ferguson, D.H., Liebert, J., 1982, PASP 94, 560 CrossRefGoogle Scholar
Hutchings, J., Cowley, A.P., 1984, PASP 96, 554 Google Scholar
Philip, A.G.D., Stock, J., 1972, Bol.Ton.Tacubaya 6, 201 Google Scholar
Pismis, P., 1972, Bol.Ton.Tacubaya 6, 197 Google Scholar
Ritter, H., Burkert, A., 1985, Proc. ESA-Workshop, ESA SP-236, 17 Google Scholar
Rupprecht, G., Bues, I., 1983, Mitt.Astron.Ges. 60, 337 Google Scholar
van Genderen, A.M., 1973, Inf.Bull.Variable Stars 815 Google Scholar