Intermediated-band photometry of late-type stars. IX - Two Hyades-like clusters

Details Intermediated-band photometry of late-type stars. IX - Two Hyades-like clusters Intermediated-band photometry of late-type stars. IX - Two Hyades-like clusters

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...234..168e&link_type=abstract

Astrophysical Journal, Part 1, vol. 234, Nov. 15, 1979, p. 168-173.

Astronomy and Astrophysics

Astrophysics

12

Giant Stars, Late Stars, Star Clusters, Stellar Spectrophotometry, K Stars, Red Giant Stars, Stellar Luminosity, Tables (Data)

Scientific paper

Observations of NGC 2423 and 2482 are discussed. NGC 2423 has a dozen early G-type to late K-type giants. Although the reddest and brightest giant needs confirmation of cluster membership, the remaining stars show a color-luminosity distribution very similar to that found previously for the Hyades group giants, and a chemical homogeneity with the Hyades group giants. A preliminary (Mv, C1)-calibration is briefly discussed. NGC 2482, which may contain the cataclysmic variable BX Pup, is slightly younger than the Hyades and NGC 2323, but the metal abundance is similar.

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