IN-SYNC. V. Stellar Kinematics and Dynamics in the Orion A Molecular Cloud

The kinematics and dynamics of young stellar populations enable us to test theories of star formation. With this aim, we continue our analysis of the SDSS-III/APOGEE IN-SYNC survey, a high-resolution near-infrared spectroscopic survey of young clusters. We focus on the Orion A star-forming region, f...

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Veröffentlicht in:	The Astrophysical journal 2017-08, Vol.845 (2), p.105
Hauptverfasser:	Da Rio, Nicola, Tan, Jonathan C., Covey, Kevin R., Cottaar, Michiel, Foster, Jonathan B., Cullen, Nicholas C., Tobin, John, Kim, Jinyoung S., Meyer, Michael R., Nidever, David L., Stassun, Keivan G., Chojnowski, S. Drew, Flaherty, Kevin M., Majewski, Steven R., Skrutskie, Michael F., Zasowski, Gail, Pan, Kaike
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ASYMMETRY Biological evolution CORRELATIONS COSMIC GASES DENSITY DISPERSIONS DISTRIBUTION EXPANSION Infrared analysis Infrared spectra Kinematics MAIN SEQUENCE STARS Molecular clouds Molecular gases MOLECULES Near infrared radiation open clusters and associations: individual (Orion Nebula Cluster, L1641) Polls & surveys RADIAL VELOCITY RESOLUTION SPECTRA Star & galaxy formation Star clusters STAR EVOLUTION Star formation stars: formation stars: kinematics and dynamics stars: pre-main sequence Stellar kinematics Stellar populations Subpopulations
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