A color-magnitude diagram for the Large Magellanic Cloud cluster NGC 1847.

Details A color-magnitude diagram for the Large Magellanic Cloud cluster NGC 1847. A color-magnitude diagram for the Large Magellanic Cloud cluster NGC 1847.

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pasp...95....5n&link_type=abstract

Publications of the Astronomical Society of the Pacific, Vol. 95, No. 563, p. 5 - 11

Astronomy and Astrophysics

Astronomy

14

C-M Diagrams:Globular Clusters, Globular Clusters:C-M Diagrams, Globular Clusters:Element Abundances, Globular Clusters:Magellanic Clouds, Magellanic Clouds:Globular Clusters

Scientific paper

Star counts to V ≍ 21 in and around the LMC cluster NGC 1847 compare well with King models. A core radius of 1.2 pc and a tidal radius of 12 pc are derived. The counts indicate that the mass of stars in the cluster brighter than MV = +1m.0 is ˜104 Msun. A color-magnitude diagram shows a well-populated main sequence and sparsely-populated but well-defined giant branch. The authors derive an age for the cluster of 25 ± 10 million years and find that it has a heavy element abundance of Z ˜ 0.01.

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