Abundances in the envelopes of massive stars undergoing mass loss

Details Abundances in the envelopes of massive stars undergoing mass loss Abundances in the envelopes of massive stars undergoing mass loss

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..230t&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, Apr. 1983, p. 230-234) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, Mar.-Apr.

Computer Science

Numerical Analysis

1

Abundance, Red Giant Stars, Stellar Envelopes, Stellar Mass Ejection, Chemical Composition, Chemical Evolution, Helium, Numerical Analysis, Stellar Evolution, Wolf-Rayet Stars

Scientific paper

The evolution of the chemical composition of the envelope of a 64 M_sun; star losing mass with the rate of ≡10-5 M_sun;/year has been studied numerically. The computations have been performed up to the core helium exhaustion stage. Mass loss rates necessary for uncovering of shells with peculiar chemical composition which is typical for OBN, WN and WC stars have been estimated.

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