The Century Survey Galactic Halo Project.: III.: A complete 4300 deg2 survey of blue horizontal branch stars in the metal-weak thick disk and inner halo

被引:47
作者
Brown, Warren R. [1 ]
Beers, Timothy C. [2 ,3 ]
Wilhelm, Ronald [4 ]
Prieto, Carlos Allende [5 ,6 ]
Geller, Margaret J. [1 ]
Kenyon, Scott J. [1 ]
Kurtz, Michael J. [1 ]
机构
[1] Smithsonian Astrophys Observ, Cambridge, MA 02138 USA
[2] Michigan State Univ, Dept Phys & Astron, Ctr Study Cosm Evolut, E Lansing, MI 48824 USA
[3] Michigan State Univ, Joint Inst Nucl Astrophys, E Lansing, MI 48824 USA
[4] Texas Tech Univ, Dept Phys, Lubbock, TX 79409 USA
[5] Univ Texas Austin, McDonald Observ, Austin, TX 78712 USA
[6] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA
关键词
Galaxy : halo; Galaxy : stellar content; stars : early type; stars : horizontal-branch;
D O I
10.1088/0004-6256/135/2/564
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a complete spectroscopic survey of 2414 2MASS-selected blue horizontal branch ( BHB) candidates selected over 4300 deg(2) 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 dv(rot)/d|Z|=-28 +/- 3.4 km s(-1) in the region |Z| < 6 kpc, and a density scale height of h(Z) = 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.
引用
收藏
页码:564 / 574
页数:11
相关论文
共 91 条
[91]   The second US Naval Observatory CCD Astrograph Catalog (UCAC2) [J].
Zacharias, N ;
Urban, SE ;
Zacharias, MI ;
Wycoff, GL ;
Hall, DM ;
Monet, DG ;
Rafferty, TJ .
ASTRONOMICAL JOURNAL, 2004, 127 (05) :3043-3059