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Spectroscopy and optical/IR photometry of the cataclysmic variable CPD-48°1577

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Abstract

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.

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Author notes

  1. A. Bruch

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

  2. R. Schoembs

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

Authors and Affiliations

  1. Dr. Remeis Sternwarte Bamberg, Astronomisches Institut der Universität Erlangen, Nürnberg, F.R.G.

    W. Wargau, A. Bruch, H. Drechsel, J. Rahe & R. Schoembs

Authors
  1. W. Wargau
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  2. A. Bruch
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  3. H. Drechsel
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  4. J. Rahe
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  5. R. Schoembs
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Additional information

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

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Wargau, W., Bruch, A., Drechsel, H. et al. Spectroscopy and optical/IR photometry of the cataclysmic variable CPD-48°1577. Astrophys Space Sci 99, 145–151 (1984). https://doi.org/10.1007/BF00650238

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  • DOI: https://doi.org/10.1007/BF00650238

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