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The chemical evolution of the Galaxy: the importance of stars with an initial mass larger than 40 M⊙

✍ Scribed by E. De Donder; D. Vanbeveren


Publisher
Elsevier Science
Year
2003
Tongue
English
Weight
159 KB
Volume
8
Category
Article
ISSN
1384-1076

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✦ Synopsis


In the present paper we investigate in how far stars with an initial mass larger than 40 M affect the chemical enrichment ( of the Galaxy. We illustrate the importance for chemical yields of a most up-to-date treatment of the various stellar wind mass loss episodes in stellar evolutionary codes and we discuss the effects of a possible supernova-like outburst prior to massive black hole formation.


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