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The asymmetry of the velocity distribution in the rotating ring in U Gem stars

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Abstract

It is shown that the non-keplerian character of the rotation of the ring of gas particles in a close binary system gives too large an amplitude of the radial velocity curve if this amplitude is determined from the positions of the emission lines of the ring.

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Authors and Affiliations

  1. Institute of Astronomy, Polish Academy of Sciences, Poland

    B. Paczyński

  2. Astronomical Observatory of the Warsaw University, Warsaw, Poland

    S. L. Piotrowski

  3. Computation Center, Polish Academy of Sciences, Poland

    W. Turski

Authors
  1. B. Paczyński
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  2. S. L. Piotrowski
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  3. W. Turski
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Paczyński, B., Piotrowski, S.L. & Turski, W. The asymmetry of the velocity distribution in the rotating ring in U Gem stars. Astrophys Space Sci 2, 254–257 (1968). https://doi.org/10.1007/BF00651569

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  • DOI: https://doi.org/10.1007/BF00651569

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