Disentangling the Galactic halo with APOGEE. I. Chemical and kinematical investigation of distinct metal-poor populations

Abstract:

We find two chemically distinct populations separated relatively cleanly in the [Fe/H]–[Mg/Fe] plane, but also distinguished in other chemical planes, among metal-poor stars (primarily with metallicities ) observed by the Apache Point Observatory Galactic Evolution Experiment (APOGEE) and analyzed for Data Release 13 (DR13) of the Sloan Digital Sky Survey. These two stellar populations show the most significant differences in their [X/Fe] ratios for the α-elements, C+ N, Al, and Ni. In addition to these populations having differing chemistry, the low metallicity high-Mg population (which we denote" the HMg population") exhibits a significant net Galactic rotation, whereas the low-Mg population (or" the LMg population") has halo-like kinematics with little to no net rotation. Based on its properties, the origin of the LMg population is likely an accreted population of stars. The HMg population shows chemistry …

Año de publicación:

2018

Keywords:

Fuente:

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