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Semi-detached binaries: The origin and present status of TU Mon, SX Cas, and DM Per

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Abstract

An attempt is made to trace back the possible progenitor systems of the Algol-type binaries TU Mon, SX Cas, and DM Per. The present characteristics are compared to the result of the evolution of 9M 0+5.4M 0. The position of the hot components in the HRD is discussed with regard to the theoretical models.

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Authors and Affiliations

  1. Astrophysical Institute, Vrije Universiteit Brussel, Belgium

    J. P. De Grève & W. Packet

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  1. J. P. De Grève
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  2. W. Packet
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De Grève, J.P., Packet, W. Semi-detached binaries: The origin and present status of TU Mon, SX Cas, and DM Per. Astrophys Space Sci 99, 313–317 (1984). https://doi.org/10.1007/BF00650255

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  • DOI: https://doi.org/10.1007/BF00650255

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