Hostname: page-component-745bb68f8f-s22k5 Total loading time: 0 Render date: 2025-01-12T15:05:56.051Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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