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

Journal Article · Thu Dec 01 04:00:00 EST 1983 · Astron. J.; (United States)

DOI:https://doi.org/10.1086/113470· OSTI ID:5512575

Smith, G H

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.

• Research Organization: Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138
• OSTI ID: 5512575
• Journal Information: Astron. J.; (United States), Journal Name: Astron. J.; (United States) Vol. 88:12; ISSN ANJOA
• Country of Publication: United States
• Language: English

Related Subjects

640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ABUNDANCE
CHEMICAL COMPOSITION
CHEMISTRY
COLOR
COSMOCHEMISTRY
CYANOGEN
DWARF STARS
GIANT STARS
OPTICAL PROPERTIES
ORGANOLEPTIC PROPERTIES
PHOTOMETRY
PHYSICAL PROPERTIES
STAR CLUSTERS
STARS