Coordinates and RI photometry of Large Magellanic Cloud carbon stars

Details Coordinates and RI photometry of Large Magellanic Cloud carbon stars Coordinates and RI photometry of Large Magellanic Cloud carbon stars

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..789c&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, July 1990, p. 789-792. Research supported by the U

Astronomy and Astrophysics

Astronomy

3

Carbon Stars, Magellanic Clouds, Stellar Luminosity, Stellar Spectrophotometry, Astronomical Photography, Near Infrared Radiation

Scientific paper

Coordinates and photoelectric RI magnitudes are given for 86 carbon stars discovered by Blanco et al. in four selected 0.12 deg sq areas of the LMC. A comparison with the photometry of Blanco et al. for carbon stars in three different fields of the LMC suggests that the luminosity distribution of the carbon stars may change from center to center in the LMC. This possibility is supported by the differences in the mean I magnitude of the carbon stars detected between the four areas studied.

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