The evolutionary status of stars with M approximately equal to or greater than 50 solar masses

Details The evolutionary status of stars with M approximately equal to or greater than 50 solar masses The evolutionary status of stars with M approximately equal to or greater than 50 solar masses

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..491t&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Aug. 1980, p. 491-494.) Soviet Astronomy Letters, vol. 6, July-Aug. 1980, p. 271-273

Astronomy and Astrophysics

Astronomy

1

Binary Stars, Hot Stars, Main Sequence Stars, Stellar Evolution, Stellar Mass, Stellar Mass Ejection, B Stars, Hertzsprung-Russell Diagram, O Stars, Stellar Envelopes, Supergiant Stars, Supernovae, Wolf-Rayet Stars

Scientific paper

The observed masses and space velocities of main-sequence stars with M equal to or greater than 50 solar masses and of some of the brightest Wolf-Rayet stars (type WN 7/WN 8) are attributed to mass exchange and supernova explosions in close binary systems. Similar arguments suggest that blue supergiants intensively shedding mass may have an envelope in common with a compact, relativistic object.

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