Kinematics of Metal-poor Stars in the Galaxy (original) (raw)
ADS
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Abstract
We discuss the kinematic properties of a sample of 1936 Galactic stars, selected without kinematic bias, and with abundances (Fe/H) is less than or equal to -0.6. The stars selected for this study all have measured radial velocities, and the majority have abundances determined from spectroscopic or narrow-/intermediate-band photometric techniques. In contrast to previous examinations of the kinematics of the metal-poor stars in the Galaxy, our sample contains large numbers of stars that are located at distances in excess of 1 kpc from the Galactic plane. Thus, a much clearer picture of the nature of the metal-deficient populations in the Galaxy can now be drawn.
Publication:
The Astrophysical Journal Supplement Series
Pub Date:
January 1995
DOI:
Bibcode:
Keywords:
- Abundance;
- Astronomical Models;
- Kinematics;
- Metallicity;
- Milky Way Galaxy;
- Radial Velocity;
- Star Distribution;
- Stellar Spectrophotometry;
- Mass Spectroscopy;
- Maximum Likelihood Estimates;
- Astrophysics;
- STARS: KINEMATICS;
- STARS: POPULATION II