Observations of clusters in the Washington system

Details Observations of clusters in the Washington system Observations of clusters in the Washington system

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86..217h&link_type=abstract

Astronomical Journal, vol. 86, Feb. 1981, p. 217-221. Research supported by the Natural Sciences and Engineering Research Counci

Astronomy and Astrophysics

Astronomy

19

Magellanic Clouds, Milky Way Galaxy, Star Clusters, Abundance, Globular Clusters, Metallic Stars, Open Clusters

Scientific paper

Three clusters in the galaxy (47 Tucanae, NGC 2243, and NGC 2158) and the NGC 2209 cluster in the Large Magellanic Cloud were observed. The Fe-CNO-sensitive FE/H (CM) abundance index of the Washington CMT 1T2 system was near that of the DDO system; 47 Tucanae and the old open cluster NGC 2243 are similar to the Fe/H (MT) of -1.2 with a significant increase in the CNO elements. It is concluded that the remote anticenter region may have a population similar to the LMC periphery since the distant anticenter cluster NGC 2158 is the most metal deficient of the intermediate age galactic clusters.

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