AGB stars in nearby galaxies

Details AGB stars in nearby galaxies AGB stars in nearby galaxies

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..848..515t&link_type=abstract

RECENT ADVANCES IN ASTRONOMY AND ASTROPHYSICS: 7th International Conference of the Hellenic Astronomical Society. AIP Conferenc

Other

Giant And Subgiant Stars, Carbon Stars, S Stars, And Related Types, Magellanic Clouds And Other Irregular Galaxies, Spiral Galaxies

Scientific paper

This study focuses on very luminous (Mbol < -6.0 mag) AGB stars with J - Ks > 1.5 mag and H - Ks > 0.4 mag in the LMC, SMC, M31, and M33 from 2MASS data. A comparison of the most luminous AGB stars detected here with previous studies shows that our sample contains mainly OH/IR stars and carbon stars. The carbon star candidates detected here are not included in existing catalogues produced from data in the optical domain, where they are not visible since they are dust-enshrouded.

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