Study of some faint clusters of the Large Magellanic Cloud

Details Study of some faint clusters of the Large Magellanic Cloud Study of some faint clusters of the Large Magellanic Cloud

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26as...41..219m&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 41, Aug. 1980, p. 219-228. In French.

Astronomy and Astrophysics

Astrophysics

Magellanic Clouds, Star Clusters, Stellar Magnitude, Hertzsprung-Russell Diagram, Microdensitometers, Red Giant Stars

Scientific paper

Twenty-two faint clusters have been studied in a northern field of the LMC. For fifteen of these clusters, the V magnitude, the B magnitude and the B-V index are tabulated; the precision of the B and V magnitudes is 0.1 and 0.2 mag, respectively. In addition, color-magnitude diagrams are presented for the fifteen clusters down to V equals 18.2 mag. It is found for a group of nine clusters that the most brilliant stars form a red giant sequence.

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