Color-Magnitude Diagrams for Five Stellar Associations in the Large Magellanic Cloud

Details Color-Magnitude Diagrams for Five Stellar Associations in the Large Magellanic Cloud Color-Magnitude Diagrams for Five Stellar Associations in the Large Magellanic Cloud

Jul 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970saosr.319.....h&link_type=abstract

SAO Special Report #319 (1970)

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17

Scientific paper

Color-magnitude arrays for five Large Magellanic Cloud stellar associations show the following features: conspicuous main sequences, a lack of cool supergiant members, a correlation of age with density, and a modest amount of reddening. One association contains an open cluster that is probably coincident in space, and another contains a Wolf-Rayet star that is probably a member. Three bright variable stars are also possible members.

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