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Massive close binaries and evolutionary synthesis of young starbursts

Published online by Cambridge University Press:  25 May 2016

Dany Dionne
Dany Dionne*
Affiliation:
Département de physique and Observatoire du mont Mégantic Université Laval, Quebec, PQ, G1K 7P4, Canada

Abstract

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With an evolutionary synthesis code, I follow the evolution of a starburst composed of massive close binaries (MCBs) and of single stars at various metallicities. Evolutionary tracks for MCBs have been developed in collaboration with D. Vanbeveren and C. de Loore. The models reproduce the observed WR/O ratio in the Magellanic Clouds.

Type
Part 5. Wolf-Rayet stars and other massive stars in starburst galaxies: the case of Wolf-Rayet galaxies (integrated spectra)
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 596 - 597
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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