Infrared photometry of globular clusters in M31

Details Infrared photometry of globular clusters in M31 Infrared photometry of globular clusters in M31

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...286..209s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 286, Nov. 1, 1984, p. 209-215.

Astronomy and Astrophysics

Astronomy

18

Andromeda Galaxy, Globular Clusters, Infrared Photometry, Infrared Spectrophotometers, Stellar Composition, Abundance, Chemical Evolution, Infrared Astronomy, Metallicity, Milky Way Galaxy, Stellar Luminosity, Stellar Magnitude

Scientific paper

Photometry of the integrated infrared light of globular clusters in the Andromeda galaxy (M31), including many with projected distances from the galaxy nucleus greater than 10 kpc, are presented. Additional data on globular clusters in NGC 205, NGC 147, and NGC 185 are included. The data obtained indicate a well-defined relation between MK and (J-K) for globular clusters in the Local Group. The use of cluster K, (J-K) as a distance indicator is discussed.

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