RI and Teff of stars in NGC 2477 (Galaz+, 1996)

Details RI and Teff of stars in NGC 2477 (Galaz+, 1996) RI and Teff of stars in NGC 2477 (Galaz+, 1996)

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..41190413g&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/119/413. Originally published in: 1996A&AS..119..413G

Other

Clusters: Open, Photometry, Effective Temperatures

Scientific paper

Trough photometric methods we have constructed the luminosity function for the southern open cluster NGC 2477 down to Mv=~12. We present R-I color-magnitude diagrams and near-infrared color-color diagrams, which allow us to separate statistically the cluster stars from the field ones, numerous because of the galactic latitude of the cluster. Our luminosity function (LF) reproduces some features obtained by other authors, namely, a dip at Mv=~7, and a probable maximum at Mv=~12. The method developed to separate cluster stars from field stars could be of interest to other astronomical problems. (1 data file).

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