The nature of the carbon stars in the galactic bulge

Details The nature of the carbon stars in the galactic bulge The nature of the carbon stars in the galactic bulge

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...202l..27a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 202, no. 1-2, Aug. 1988, p. L27-L29.

Astronomy and Astrophysics

Astrophysics

23

Carbon Stars, Galactic Bulge, Stellar Evolution, Stellar Spectrophotometry, Asymptotic Giant Branch Stars, Binary Stars, Color-Magnitude Diagram, Infrared Photometry, Mass Transfer, Star Formation

Scientific paper

Infrared photometry of carbon stars recently found in the direction of the galactic bulge shows that they actually belong to the bulge population and that they are intrinsically faint, metal rich objects. The conventional mechanism for carbon-star formation is excluded in their case, and another mixing process is required, although they might also have been enriched in carbon through mass transfer in a binary system.

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