
Chemodynamics of the Milky Way
2014; EDP Sciences; Volume: 564; Linguagem: Inglês
10.1051/0004-6361/201323038
ISSN1432-0746
AutoresF. Anders, C. Chiappini, B. X. Santiago, H. J. Rocha–Pinto, L. Girardi, L. N. da Costa, M. A. G. Maia, Matthias Steinmetz, Ivan Minchev, M. Schultheis, C. Boeche, A. Miglio, J. Montalbán, Donald P. Schneider, Timothy C. Beers, Kátia Cunha, Carlos Allende Prieto, E. Balbinot, Dmitry Bizyaev, D. E. Brauer, J. Brinkmann, Peter M. Frinchaboy, A. E. García Pérez, Michael Hayden, Fred Hearty, Jon A. Holtzman, Jennifer A. Johnson, Karen Kinemuchi, Steven R. Majewski, Elena Malanushenko, Viktor Malanushenko, David L. Nidever, R. W. O’Connell, Kaike Pan, A. C. Robin, Ricardo P. Schiavon, Matthew Shetrone, M. F. Skrutskie, Verne V. Smith, Keivan G. Stassun, Gail Zasowski,
Tópico(s)Astronomy and Astrophysical Research
ResumoContext. The Apache Point Observatory Galactic Evolution Experiment (APOGEE) features the first multi-object high-resolution fiber spectrograph in the near-infrared ever built, thus making the survey unique in its capabilities: APOGEE is able to peer through the dust that obscures stars in the Galactic disc and bulge in the optical wavelength range. Here we explore the APOGEE data included as part of the Sloan Digital Sky Survey's 10th data release (SDSS DR10).
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