The HR 1614 moving group - Evidence from DDO photometry that it contains cyanogen-rich stars

Details The HR 1614 moving group - Evidence from DDO photometry that it contains cyanogen-rich stars The HR 1614 moving group - Evidence from DDO photometry that it contains cyanogen-rich stars

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aj.....88.1775s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 88, Dec. 1983, p. 1775-1783.

Astronomy and Astrophysics

Astronomy

15

Abundance, Cyanogen, Star Clusters, Stellar Color, Stellar Motions, Ubv Spectra, Dwarf Stars, Giant Stars, Metallicity, Milky Way Galaxy, Stellar Spectrophotometry

Scientific paper

DDO photometry is presented for a number of giants and dwarfs suggested by Eggen to belong to the HR 1614 moving group. It is found that the colors of many of these stars are similar to those of the super-metal-rich stars. There are many more strong-cyanogen stars among Eggen's suggested group members than would be expected among a randomly collected sample of field stars, and on this basis it is suggested that the HR 1614 group does in fact represent a sample of related stars.

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