Theoretical evolution of massive stellar aggregates

Details Theoretical evolution of massive stellar aggregates Theoretical evolution of massive stellar aggregates

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...124...71v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 124, no. 1, July 1983, p. 71-76.

Astronomy and Astrophysics

Astrophysics

11

B Stars, O Stars, Star Clusters, Stellar Evolution, Wolf-Rayet Stars, Binary Stars, Hertzsprung-Russell Diagram, Mass Distribution, Stellar Mass, Time Functions

Scientific paper

Evolutionary computations of massive single stars and of massive binaries are employed to model the evolution of massive stellar aggregates. An initial mass function (IMF) is defined for the mass distribution of aggregates, which is found to increase at a lower rate than that for the galactic IMF. The aggregate IMF is applied to predicting the number of WR, O, and B0-B1 stars that would appear in an aggregate as a function of time.

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