Evolution and mass loss of AGB stars.

Details Evolution and mass loss of AGB stars. Evolution and mass loss of AGB stars.

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996asthe..89..382h&link_type=abstract

Astronomical Herald, Vol. 89, No. 9, p. 382 - 387

Astronomy and Astrophysics

Astronomy

Agb Stars: Stellar Evolution, Agb Stars: Mass Loss

Scientific paper

Asymptotic giant branch is the final stage of stellar evolution of low- and intermediate-mass stars. An AGB star is a cool giant with a degenerate core of carbon and oxygen, which is surrounded by a thin helium shell and a large outer hydrogen envelope. Mass loss is commonly seen in the evolved AGB stars, playing a dominant role in the AGB evolution. The AGB evolution with mass loss is briefly reviewed on the basis of recent observational results.

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