Photometric study of the Southern open clusters NGC 5316 and NGC 6214

Details Photometric study of the Southern open clusters NGC 5316 and NGC 6214 Photometric study of the Southern open clusters NGC 5316 and NGC 6214

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....94.1237p&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 94, Nov. 1987, p. 1237-1243. Research supported by the Universidad de Chile and NSER

Astronomy and Astrophysics

Astronomy

5

Astronomical Photometry, Open Clusters, Color-Magnitude Diagram, Electrophotometry, Interstellar Extinction, Red Giant Stars, Southern Sky, Ubv Spectra

Scientific paper

Based on UBV photoelectric photometry, the individual reddenings of cluster stars in NGC 5316 and NGC 6124 were derived, and a fitting to an evolved sequence was performed on the reddening-free colors and magnitudes of cluster members. For NGC 5316, an average distance modulus of 10.34 + or - 0.07, an E(B-V) value of 0.34 + or - 0.04 s.d., and an age of about 1.2 x 10 to the 8th yr were found. For NGC 6124, an E(B-V) value of 0.80 + or - 0.06 s.d., an average distance modulus of 8.75 + or - 0.04, and an age of about 1.0 x 10 to the 8th yr are determined. The present color excesses and distance moduli are, in general, greater than previous values.

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