The open cluster NGC 2204

Details The open cluster NGC 2204 The open cluster NGC 2204

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86..237d&link_type=abstract

Astronomical Journal, vol. 86, Feb. 1981, p. 237-241.

Astronomy and Astrophysics

Astronomy

20

Abundance, Giant Stars, Open Clusters, Stellar Spectrophotometry, Cyanogen, Dwarf Stars, Electrophotometers, Metals, Red Giant Stars, Stellar Luminosity, Stellar Magnitude, Stellar Mass, Stellar Temperature

Scientific paper

Photoelectric photometry in the intermediate-band DDO system and the wideband Cousins VRI system is presented for representative giants in the old open cluster NGC 2204. The metal-poor character of the cluster, suggested by previous UBV photometry, is confirmed and an average cyanogen anomaly of -0.047 + or - 0.009 mag (m.e.) is derived. There are several stars in NGC 2204 which may have unusual surface compositions.

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