CCD photometry of the Large Magellanic Cloud cluster NGC 1866 - Observational results

Details CCD photometry of the Large Magellanic Cloud cluster NGC 1866 - Observational results CCD photometry of the Large Magellanic Cloud cluster NGC 1866 - Observational results

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apjs...71...25b&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 71, Sept. 1989, p. 25-46.

Astronomy and Astrophysics

Astrophysics

59

Astronomical Photometry, Globular Clusters, Magellanic Clouds, Stellar Evolution, Charge Coupled Devices, Color-Magnitude Diagram, Giant Stars, Star Distribution, Tables (Data)

Scientific paper

New observational evidence for evolving stars in the LMC cluster NGC 1866 is reported and discussed. Assuming Y = 0.28 and Z = 0.02 for the cluster, the data agree with theoretical prescriptions for a cluster age of 1.1 x 10 to the 8th yr. A cluster reddening e(B-V) = 0.06 appears to be supported by the data, together with a true distance modulus of 18.6 mag.

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