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The evolution of 1.40Mθpure He star

✍ Scribed by G. Shaviv; N. Vidal


Book ID
104863458
Publisher
Springer Netherlands
Year
1972
Tongue
English
Weight
537 KB
Volume
15
Category
Article
ISSN
0004-640X

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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