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The halo metallicity distribution

Published online by Cambridge University Press:  07 August 2017

J. B. Laird ,
B. W. Carney  and
D. W. Latham
J. B. Laird
Affiliation:
Bowling Green State University Department of Physics and Astronomy Bowling Green, OH 43403 USA
B. W. Carney
Affiliation:
University of North Carolina Department of Physics and Astronomy CB 3255 Phillips Hall Chapel Hill, NC 27599–3255 USA
D. W. Latham
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden Street Cambridge, MA 02138 USA

Extract

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The field dwarf sample is from the original Carney-Latham survey plus its recent extension to about 500 additional stars, a total of about 1450 stars. We have chosen a conservative criterion to isolate halo stars, namely retrograde orbits in the Galaxy, to minimize contamination by thin and thick disk stars, giving a halo sample of 144 stars.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 443
Copyright
Copyright © Kluwer