The population of young stars in Orion A: X-rays and IR properties.

Details The population of young stars in Orion A: X-rays and IR properties. The population of young stars in Orion A: X-rays and IR properties.

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cfdd.confe.177p&link_type=abstract

Chandra's First Decade of Discovery, Proceedings of the conference held 22-25 September, 2009 in Boston, MA. Edited by Scott Wo

Physics

Stars And Star Formation

Scientific paper

Stars in the very early stages of their formation are characterized by strong IR excess and X-rays emission. We present the results of the survey of Orion A in both IR and X-rays obtained with Spitzer and XMM-Newton observatories. We study the SED Class of the Young Stellar Objects (YSOs) population using IR colors from 2MASS + Spitzer (IRAC & MIPS) and by means of X-rays luminosities and plasma temperatures. We discuss clustering properties and spatial segregation among different IR class YSOs in order to track the formation history.

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