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Comments on V505 mon: One of the most massive binaries

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Abstract

From a discussion of the results or V505 Mon, we conclude that the spectral types contradict other parameters in the HR diagram.

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References

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Authors and Affiliations

  1. Astrophysical Institute, Vrije Universiteit Brussel, Brussels, Belgium

    J. P. De Greve (Research Associate FKFO, Belgium), C. Doom, P. Hellings, W. Packet & R. Stagni (Asiago Astrophysical Observatory, Asiago (Vicenza), Italy)

  2. University of Messina, Italy

    A. Mammano

Authors
  1. J. P. De Greve
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  2. C. Doom
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  3. P. Hellings
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  4. W. Packet
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  5. R. Stagni
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  6. A. Mammano
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De Greve, J.P., Doom, C., Hellings, P. et al. Comments on V505 mon: One of the most massive binaries. Astrophys Space Sci 95, 215–217 (1983). https://doi.org/10.1007/BF00661176

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  • DOI: https://doi.org/10.1007/BF00661176

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