Fundamental parameters of the open cluster NGC 2567

Details Fundamental parameters of the open cluster NGC 2567 Fundamental parameters of the open cluster NGC 2567

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986aj.....91..326c&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 91, Feb. 1986, p. 326-337. Research supported by CONICOR and CONICET.

Astronomy and Astrophysics

Astronomy

30

Astronomical Photometry, Open Clusters, Red Giant Stars, Stellar Composition, Color-Color Diagram, Distance, Electrophotometry, Interstellar Extinction, Metallicity, Stellar Color, Ubv Spectra

Scientific paper

New photoelectric UBV photometry of 164 stars brighter than V = 14.6 as well as DDO and CMT(1)T(2) photometry of five red stars in the open cluster NGC 2567 are presented and discussed. By using both color-magnitude and color-color diagrams, 81 stars (including three red giants) are found to be cluster members and 15 stars to be probable members. A foreground reddening E (B - V) = 0.13 mag, a distance modulus V(0) - M(v) 11.05 mag (d = 1620 pc), and an age of 2.9 x 10 to the 8th yr have been derived. Assuming that the metal abundance of the red giants is representative of that of the whole cluster, NGC 2567 appears to have a nearly solar composition.

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