SDSS J192339.70+375102.6 , the SIMBAD biblio

2010AJ....140..500C - Astron. J., 140, 500-509 (2010/August-0)

Metallicity and kinematic distributions of red horizontal-branch stars from the SDSS survey.

CHEN Y.Q., ZHAO G., ZHAO J.K., XUE X.X. and SCHUSTER W.J.

Abstract (from CDS):

On the basis of a recently derived color-metallicity relation and stellar parameters from the Sloan Digital Sky Survey Data Release 7 spectroscopic survey, a large sample of red horizontal-branch (RHB) candidates have been selected to serve as standard candles. The metallicity and kinematic distributions of these stars indicate that they mainly originate from the thick-disk and the halo populations. The typical thick disk is characterized by the first group peaking at [Fe/H] ∼ -0.6, Vrot∼ 170 km/s with a vertical scale height around|Z| ∼ 1.2 kpc, while stars with [Fe/H] < -0.9 are dominated by the halo population. Two sub-populations of the halo are suggested by the RHB stars peaking at [Fe/H] ∼ -1.3: one component with Vrot> 0 km/s (Halo I) shows a sign of metallicity gradient in the [Fe/H] versus |Z| diagram, while the other with Vrot< 0 km/s (Halo II) does not. The Halo I mainly clumps at the inner halo with R < 10 kpc and the Halo II comes both from the inner halo with R < 10 kpc and the outer halo with R > 10 kpc based on the star distribution in the R versus|Z| diagram.

Abstract Copyright:

Journal keyword(s): Galaxy: disk - Galaxy: halo - Galaxy: kinematics and dynamics - stars: horizontal-branch

VizieR on-line data: <Available at CDS (J/AJ/140/500): table1.dat>

Simbad objects: 4867

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2019.11.14-23:51:57

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