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Spectroscopy and Optical/IR Photometry of the Cataclysmic Variable CPD-48° 1577***

Published online by Cambridge University Press:  12 April 2016

W. Wargau ,
A. Bruch ,
H. Drechsel ,
J. Rahe  and
R. Schoembs
W. Wargau
Affiliation:
Dr. Remeis Sternwarte Bamberg, Astronomisches Institut der Universität Erlangen, Nürnberg, F.R.G.
A. Bruch
Affiliation:
Dr. Remeis Sternwarte Bamberg, Astronomisches Institut der Universität Erlangen, Nürnberg, F.R.G.
H. Drechsel
Affiliation:
Dr. Remeis Sternwarte Bamberg, Astronomisches Institut der Universität Erlangen, Nürnberg, F.R.G.
J. Rahe
Affiliation:
Dr. Remeis Sternwarte Bamberg, Astronomisches Institut der Universität Erlangen, Nürnberg, F.R.G.
R. Schoembs
Affiliation:
Dr. Remeis Sternwarte Bamberg, Astronomisches Institut der Universität Erlangen, Nürnberg, F.R.G.

Abstract

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The photometric variability of CPD-48°1577 in the optical and IR ranges is discussed. The structure and variation of prominent emission line profiles are investigated. An estimate of the distance is given.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 80: Double Stars, Physical Properties and Generic Relations , 1984 , pp. 145 - 151
Copyright
Copyright © Reidel 1984

Footnotes

a

Astronomisches Institut der Westfälischen Wilhelms-Universität Münster, F.R.G.

b

Institut für Astronomie und Astrophysik der Universität München, F.R.G.

*

Paper presented at the Lembang-Bamberg IAU Colloquium No. 80 on ‘Double Stars: Physical Properties and Generic Relations', held at Bandung, Indonesia, 3-7 June, 1983.

**

Based on data collected at the European Southern Observatory in Chile.

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