SDSS J124339.00+595513.4 , the SIMBAD biblio

2010ApJ...725L.186D - Astrophys. J., 725, L186-L190 (2010/December-3)

Observational evidence from SDSS for a merger origin of the Milky Way's thick disk.

DIERICKX M., KLEMENT R., RIX H.-W. and LIU C.

Abstract (from CDS):

We test four competing models that aim to explain the nature of stars in spiral galaxies that are well away (>1 kpc) from the midplane, the so-called thick disk: the stars may have gotten there through orbital migration, through satellite mergers and accretion, or through heating of pre-existing thin disk stars. The eccentricity distribution of thick disk stars has recently been proposed as a diagnostic to differentiate between these mechanisms. Drawing on SDSS data release 7, we have assembled a sample of 31,535 G-dwarfs with six-dimensional phase-space information and metallicities and have derived the orbital eccentricities for them. Comparing the resulting eccentricity distributions, p(e|z), with these particular simulations, we find that: (1) the observed p(e|z) is inconsistent with that predicted by orbital migration only, as there are more observed stars of high and of very low eccentricity; (2) simulations in which the thick disk is made predominantly through heating a pre-existing thin disk are also inconsistent, as they predict more high-eccentricity stars than observed; (3) the observed p(e|z) fits well with a "gas-rich merger" scenario, where most thick disk stars were born in situ. Further modeling could explore whether the data-simulation inconsistencies found here for the first three cases actually rule out the qualitative scenarios underlying these simulations.

Abstract Copyright:

Journal keyword(s): galaxies: individual: Milky Way - Galaxy: evolution - Galaxy: kinematics and dynamics - Galaxy: structure

VizieR on-line data: <Available at CDS (J/ApJ/725/L186): table2.dat>

Simbad objects: 31530

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2019.11.12-23:27:14

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