Abstract
We present a complete spectroscopic survey of 2414 2MASS-selected blue horizontal branch (BHB) candidates selected over 4300 deg2 of the sky. We identify 655 BHB stars in this non-kinematically selected sample. We calculate the luminosity function of field BHB stars, and find evidence for very few hot BHB stars in the field. The BHB stars located at a distance from the Galactic plane |Z| < 4 kpc trace what is clearly a metal-weak thick disk population, with a mean metallicity of [Fe/H] = -1.7, a rotation velocity gradient of dvrot/d|Z| = -28 3.4 km s-1 in the region |Z| < 6 kpc, and a density scale height of hZ = 1.26 0.1 kpc. The BHB stars located at 5 < |Z| < 9 kpc are a predominantly inner-halo population, with a mean metallicity of [Fe/H] = -2.0 and a mean Galactic rotation of -4 31 km s-1. We infer the density of halo and thick disk BHB stars is 104 37 kpc-3 near the Sun, and the relative normalization of halo to thick-disk BHB stars is 4 1% near the Sun.
| Original language | English |
|---|---|
| Pages (from-to) | 564-574 |
| Number of pages | 11 |
| Journal | Astronomical Journal |
| Volume | 135 |
| Issue number | 2 |
| DOIs | |
| State | Published - Feb 1 2008 |
Keywords
- Galaxy: halo
- Galaxy: stellar content
- Stars: early type
- Stars: horizontal-branch
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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