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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.

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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