Identifying Sagittarius Stream Stars by Their APOGEE Chemical Abundance Signatures

Sten Hasselquist (1) , Jeffrey Carlin , Jon Holtzman (2) , Matthew Shetrone (3) , Christian Hayes , Katia Cunha , Verne Smith (4) , Rachael Beaton , Jennifer Sobeck (5) , Carlos Allende Prieto , Steven Majewski , Borja Anguiano , Dmitry Bizyaev , D. García-Hernández , Richard Lane , Kaike Pan , David Nidever (6, 4) , José Gregorio Fernández-Trincado (7, 8, 9) , John Wilson (10) , Olga Zamora (11)

1 University of Utah
2 New Mexico State University
3 McDonald Observatory
4 NOAO - National Optical Astronomy Observatory
5 University of Washington [Seattle]
6 MSU - Montana State University
7 UTINAM - Univers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213)
8 INCT - Instituto de Astronomia y ciencias Planetarias de Atacama
9 Universidad de Concepción - University of Concepcion [Chile]
10 University of Virginia
11 ULL - Universidad de La Laguna [Tenerife - SP]

Domaines: Astrophysique [astro-ph]

Sten Hasselquist, Jeffrey Carlin, Jon Holtzman, Matthew Shetrone, Christian Hayes, et al.. Identifying Sagittarius Stream Stars by Their APOGEE Chemical Abundance Signatures. The Astrophysical Journal, 2019, 872 (1), pp.58. ⟨10.3847/1538-4357/aafdac⟩. ⟨hal-02738750⟩