Comments on V505 MON - One of the most massive binaries

Details Comments on V505 MON - One of the most massive binaries Comments on V505 MON - One of the most massive binaries

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..95..215d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 95, no. 1, Sept. 1983, p. 215-217.

Astronomy and Astrophysics

Astrophysics

1

Binary Stars, Stellar Evolution, Stellar Mass, Supermassive Stars, Hertzsprung-Russell Diagram, Mass To Light Ratios, Radii, Stellar Spectra

Scientific paper

The results of Stagni et al. (1982) for the dimensions of V505 Mon are discussed with regard to stellar and close binary evolution. The HRD position of each component is determined and compared to possible positions of theoretical stars of comparable mass in the HRD according to various evolutionary computations. These theoretical components indicate masses for the components which are incompatical with the masses derived by Stagni et al. and are also impossible for physical reasons.

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