Tracing Chemical Evolution Over The Extent Of The Milky Way's Disk With Apogee Red Clump Stars

Autor: Annie C. Robin, Jian Ge, Steven R. Majewski, Howard Brewington, Kaike Pan, Peter M. Frinchaboy, Matthew Shetrone, Moses Marchante, David L. Nidever, Jonathan C. Bird, Ivan Minchev, Cristina Chiappini, Jo Bovy, Dmitry Bizyaev, Jon A. Holtzman, John C. Wilson, Elena Malanushenko, Karen Kinemuchi, Diane Feuillet, Brett H. Andrews, Donald P. Schneider, Audrey Simmons, Katia Cunha, Hans-Walter Rix, Timothy C. Beers, Gail Zasowski, Viktor Malanushenko, Verne V. Smith, Olga Zamora, Jennifer A. Johnson, Garrett Ebelke, Jennifer Sobeck, Robert W. O'Connell, D. A. García-Hernández, Carlos Allende Prieto, Szabolcs Mészáros, Ana G. Pérez, Michael F. Skrutskie, Ricardo P. Schiavon, David H. Weinberg, Friedrich Anders, Daniel Oravetz, Michael R. Hayden
Přispěvatelé: Univers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) (UTINAM), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC)
Jazyk: angličtina
Rok vydání: 2014
Předmět:
Zdroj: The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2014, 796, 1, pp.38. ⟨10.1088/0004-637X/796/1/38⟩
ISSN: 0004-637X
1538-4357
DOI: 10.1088/0004-637X/796/1/38⟩
Popis: We employ the first two years of data from the near-infrared, high-resolution SDSS-III/APOGEE spectroscopic survey to investigate the distribution of metallicity and alpha-element abundances of stars over a large part of the Milky Way disk. Using a sample of ~10,000 kinematically-unbiased red-clump stars with ~5% distance accuracy as tracers, the [alpha/Fe] vs. [Fe/H] distribution of this sample exhibits a bimodality in [alpha/Fe] at intermediate metallicities, -0.9
Comment: 18 pages, 17 figures. Accepted for publication in ApJ
Databáze: OpenAIRE