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

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

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..99..313d&link_type=abstract

(International Astronomical Union, Colloquium on Double Stars, Physical Properties and Generic Relations, 80th, Bandung, Indones

Astronomy and Astrophysics

Astrophysics

4

Binary Stars, Stellar Evolution, Stellar Mass, Mass To Light Ratios, Mass Transfer, Stellar Models

Scientific paper

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 9
M0 + 5.4 M0. The position of the hot components in
the HRD is discussed with regard to the theoretical models.

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