Carbon Stars in the Sagittarius Dwarf Galaxy

Details Carbon Stars in the Sagittarius Dwarf Galaxy Carbon Stars in the Sagittarius Dwarf Galaxy

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999iaus..192..136w&link_type=abstract

The stellar content of Local Group galaxies, Proceedings of the 192nd symposium of the International Astronomical Union held in

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13

Scientific paper

The luminosities of carbon stars in the Sagittarius Dwarf are derived from infrared photometry and compared with those of carbon stars in other galaxies. Several of them are large amplitude, probably Mira, variables and one shows obscuration episodes characteristic of galactic carbon stars with moderate mass-loss rates, e.g. R For and R Lep. These variables are more like those found in the Magellanic Clouds than in dwarf spheroidals.

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