Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...224...73a&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 224, no. 1-2, Oct. 1989, p. 73-85.
Astronomy and Astrophysics
Astronomy
86
H Ii Regions, Local Group (Astronomy), Metallicity, Star Distribution, Stellar Evolution, Wolf-Rayet Stars, Magellanic Clouds, O Stars, Solar Neighborhood, Star Formation Rate, Stellar Mass
Scientific paper
Synthetic populations of massive stars are used to study the evolution of WR star populations at solar and SMC metallicities. The effects of different star formation scenarios and IMF slopes are examined. Consideration is given to an instantaneous burst and a constant star formation rate in which massive stars are continuously replaced. Results of the synthetic population models are presented, including the behavior of the synthesized number ratios of WR to O stars and WC to WR stars are studied as a function of time.
Arnault Ph.
Kunth Daniel
Schild Hans
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