Chemodynamics of the Milky Way I. The first year of APOGEE data

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20165103151977
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[1] [1,Anders, F.
[2] 1,Chiappini, C.
[3] 3,Santiago, B.X.
[4] Rocha-Pinto, H.J.
[5] 3,Girardi, L.
[6] 3,Da Costa, L.N.
[7] 3,Maia, M.A.G.
[8] Steinmetz, M.
[9] Minchev, I.
[10] Schultheis, M.
[11] Boeche, C.
[12] Miglio, A.
[13] Montalbán, J.
[14] 12,Schneider, D.P.
[15] 14,Beers, T.C.
[16] 7,Cunha, K.
[17] Allende Prieto, C.
[18] 3,Balbinot, E.
[19] Bizyaev, D.
[20] Brauer, D.E.
[21] Brinkmann, J.
[22] Frinchaboy, P.M.
[23] García Pérez, A.E.
[24] Hayden, M.R.
[25] 20,Hearty, F.R.
[26] Holtzman, J.
[27] Johnson, J.A.
[28] Kinemuchi, K.
[29] Majewski, S.R.
[30] Malanushenko, E.
[31] Malanushenko, V.
[32] Nidever, D.L.
[33] O'Connell, R.W.
[34] Pan, K.
[35] Robin, A.C.
[36] Schiavon, R.P.
[37] Shetrone, M.
[38] Skrutskie, M.F.
[39] Smith, V.V.
[40] Stassun, K.
[41] Zasowski, G.
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| 1600年 / EDP Sciences卷 / 564期
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Context. 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). Aims. The goal of this paper is to a) investigate the chemo-kinematic properties of the Milky Way disc by exploring the first year of APOGEE data; and b) to compare our results to smaller optical high-resolution samples in the literature; as well as results from lower resolution surveys such as the Geneva-Copenhagen Survey (GCS) and the RAdial Velocity Experiment (RAVE). Methods. We select a high-quality (HQ) sample in terms of chemistry (amounting to around 20 000 stars) and; after computing distances and orbital parameters for this sample; we employ a number of useful subsets to formulate constraints on Galactic chemical and chemodynamical evolution processes in the solar neighbourhood and beyond (e.g; metallicity distributions - MDFs; α/Fe; vs; Fe/H; diagrams; and abundance gradients). Results. Our red giant sample spans distances as large as 10 kpc from the Sun. Given our chemical quality requirements; most of the stars are located between 1 and 6 kpc from the Sun; increasing by at least a factor of eight the studied volume with respect to the most recent chemodynamical studies based on the two largest samples obtained from RAVE and the Sloan Extension for Galactic Understanding and Exploration (SEGUE). We find remarkable agreement between the MDF of the recently published local (d © ESO 2014;
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