A UBV and DDO astrophysical study of the open cluster NGC 3532

Details A UBV and DDO astrophysical study of the open cluster NGC 3532 A UBV and DDO astrophysical study of the open cluster NGC 3532

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.235.1129c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 235, Dec. 15, 1988, p. 1129-1139. Research supported by

Mathematics

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16

Astronomical Photometry, Electrophotometry, Star Clusters, Ubv Spectra, Cyanogen, Hertzsprung-Russell Diagram, Interstellar Extinction, Red Giant Stars, Star Distribution, Stellar Color

Scientific paper

Photoelectric observations in the UBV and DDO systems have been obtained for 12 stars on the red giant branch of NGC 3532. A mean reddening E(B-V) = 0.07 + or - 0.02 has been determined from the red cluster giants. The results show nearly solar metallicity for NGC 3532, and imply that most of the stars are red giants in the core helium burning stage of evolution.

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