Evolution of Massive Stars: Observational Evidence

Author
Abstract

The stellar population of O, B and Wolf-Rayet stars within 3 kpc of the Sun is discussed. In addition to providing observational data for comparison with evolutionary models, the observations suggest a galactic gradient in the initial mass function of these stars. Differences in the massive stellar population between the Large and Small Magellanic Cloud are starting to appear. Understanding these differences will provide important insight into the evolution of galaxies.

Year of Conference
1985
Start Page or Article ID
79-88
Publisher
Springer Netherlands
Conference Location
Dordrecht
ISBN Number
978-94-009-5478-6
DOI
10.1007/978-94-009-5478-6_11
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Publication Status
JILA PI
JILA Topics
Conference Proceedings