Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..747f&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, July-Aug. 1988, p. 747-752. In Russian.
Astronomy and Astrophysics
Astronomy
Asymptotic Giant Branch Stars, Carbon, Oxygen, Stellar Cores, Stellar Mass Ejection, Stellar Evolution, Stellar Luminosity, Supernovae
Scientific paper
The luminosity of some asymptotic giant branch stars in the SMC is high enough that the final phase of the evolution may be a supernova burst. This type of star is not found in the LMC. The comparison of theoretical and observed luminosity distributions of stars in the Magellanic clouds shows that the mass loss rate of high-luminosity asymptotic giant branch stars in the LMC is about one order of magnitude larger than in the SMC.
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