Carbon stars possibly associated with clusters in the Large Magellanic Cloud

Details Carbon stars possibly associated with clusters in the Large Magellanic Cloud Carbon stars possibly associated with clusters in the Large Magellanic Cloud

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...221..586s&link_type=abstract

Astrophysical Journal, Part 1, vol. 221, Apr. 15, 1978, p. 586, 587.

Mathematics

Probability

4

Carbon Stars, Giant Stars, Magellanic Clouds, Star Clusters, Astronomical Catalogs, Galactic Evolution, Open Clusters, Probability Distribution Functions, Statistical Analysis, Stellar Evolution

Scientific paper

A list is given of nine carbon stars which fall in or very near clusters
in the Large Magellanic Cloud (LMC). Statistical arguments indicate that
at least several of these may be physical members. The low frequency of
occurrence of carbon stars in LMC open clusters conforms with the
apparent rarity of this phenomenon in our own Galaxy.

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