THE APOGEE RED-CLUMP CATALOG: PRECISE DISTANCES, VELOCITIES, AND HIGH-RESOLUTION ELEMENTAL ABUNDANCES OVER A LARGE AREA OF THE MILKY WAY'S DISK

The Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution near-infrared spectroscopic survey covering all of the major components of the Galaxy, including the dust-obscured regions of the inner Milky Way disk and bulge. Here we prese...

Celý popis

Uloženo v:
Podrobná bibliografie
Vydáno v:The Astrophysical journal Ročník 790; číslo 2; s. 127 - 21
Hlavní autoři: Bovy, Jo, Nidever, David L., Rix, Hans-Walter, Girardi, Léo, Zasowski, Gail, Chojnowski, S. Drew, Holtzman, Jon, Epstein, Courtney, Frinchaboy, Peter M., Hayden, Michael R., Rodrigues, Thaíse S., Majewski, Steven R., Johnson, Jennifer A., Pinsonneault, Marc H., Stello, Dennis, Allende Prieto, Carlos, Andrews, Brett, Basu, Sarbani, Beers, Timothy C., Bizyaev, Dmitry, Burton, Adam, Chaplin, William J., Cunha, Katia, Elsworth, Yvonne, García, Rafael A., García-Herńandez, Domingo A., García Pérez, Ana E., Hearty, Fred R., Hekker, Saskia, Kallinger, Thomas, Kinemuchi, Karen, Koesterke, Lars, Mészáros, Szabolcs, Mosser, Benoît, O'Connell, Robert W., Oravetz, Daniel, Pan, Kaike, Robin, Annie C., Schiavon, Ricardo P., Schneider, Donald P., Schultheis, Mathias, Serenelli, Aldo, Shetrone, Matthew, Silva Aguirre, Victor, Simmons, Audrey, Skrutskie, Michael, Smith, Verne V., Stassun, Keivan, Weinberg, David H., Wilson, John C., Zamora, Olga
Médium: Journal Article
Jazyk:angličtina
Vydáno: United States American Astronomical Society 01.08.2014
Témata:
ABUNDANCE
Apogees
APPROXIMATIONS
Astrophysics
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
COLOR
Disks
DISTANCE
DUSTS
GALACTIC EVOLUTION
Glass transition temperature
GRAVITATION
ISOCHRONOUS CYCLOTRONS
LUMINOSITY
Mathematical models
METALLICITY
MILKY WAY
PHOTOMETRY
Physics
PROPER MOTION
Sciences of the Universe
SPACE DEPENDENCE
SPECTRA
STAR EVOLUTION
Stars
SUN
SURFACES
Galaxy: stellar content
Galaxy: disk
Galaxy: structure
stars: general
Galaxy: abundances
stars: distances
ISSN:0004-637X, 1538-4357
On-line přístup:Získat plný text
Tagy: Přidat tag
Žádné tagy, Buďte první, kdo vytvoří štítek k tomuto záznamu!
Popis
Shrnutí:The Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution near-infrared spectroscopic survey covering all of the major components of the Galaxy, including the dust-obscured regions of the inner Milky Way disk and bulge. Here we present a sample of 10,341 likely red-clump stars (RC) from the first two years of APOGEE operations, selected based on their position in color- metallicity-surface-gravity-effective-temperature space using a new method calibrated using stellar evolution models and high-quality asteroseismology data. The narrowness of the RC locus in color-metallicity-luminosity space allows us to assign distances to the stars with an accuracy of 5%-10%. The sample extends to typical distances of about 3 kpc from the Sun, with some stars out to 8 kpc, and spans a volume of approximately 100 kpc super(3) over 5 kpc [lap] R [lap] 14 kpc, |Z| [lap] 2 kpc, and -15[degrees] [lap] Galactocentric azimuth [lap] 30[degrees]. The APOGEE red-clump (APOGEE-RC) catalog contains photometry from the Two Micron All Sky Survey, reddening estimates, distances, line-of-sight velocities, stellar parameters and elemental abundances determined from the high-resolution APOGEE spectra, and matches to major proper motion catalogs. We determine the survey selection function for this data set and discuss how the RC selection samples the underlying stellar populations. We use this sample to limit any azimuthal variations in the median metallicity within the approximately 45[degrees] azimuthal region covered by the current sample to be [< or =, slant]0.02 dex, which is more than an order of magnitude smaller than the radial metallicity gradient. This result constrains coherent non-axisymmetric flows within a few kiloparsecs from the Sun.
Bibliografie:ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:0004-637X
1538-4357
DOI:10.1088/0004-637X/790/2/127