Three luminous carbon stars in the Large Magellanic Cloud

Details Three luminous carbon stars in the Large Magellanic Cloud Three luminous carbon stars in the Large Magellanic Cloud

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...219..452r&link_type=abstract

Astrophysical Journal, Part 1, vol. 219, Jan. 15, 1978, p. 452, 453. Research supported by the National Research Council of Can

Astronomy and Astrophysics

Astrophysics

4

Abundance, Carbon Stars, Magellanic Clouds, Variable Stars, Carbon 13, Emission Spectra, Mira Variables, Radial Velocity, Stellar Luminosity, Stellar Spectra

Scientific paper

The properties of three very luminous carbon stars in the Large
Magellanic Cloud are discussed. Two of the three are rather blue, with
(R-I) values of about 0.88, and exhibit significant amounts of C-13 in
their spectra. The third is the first carbon Mira to be found in the
LMC.

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