Highlights from the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

Güdel, M.; Arzner, K.; Audard, M.; Bouvier, J.; Briggs, K.; Dougados, C.; Feigelson, E.; Franciosini, E.; Glauser, A.; Grosso, N.; Guieu, S.; Ménard, F.; Micela, G.; Monin, J.; Montmerle, T.; Padgett, D.; Palla, F.; Pillitteri, I.; Preibisch, T.; Rebull, L.; Scelsi, L.; Silva, B.; Skinner, S.; Stelzer, B.; Telleschci, A.

14th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
ASP Conference Series, Vol. 384
Proceedings of the conference held 5-10 November, 2006, at the Spitzer Science Center and Michelson Science Center, Pasadena, California, USA.
Edited by Gerard van Belle., p.65 (2008)

Abstract
The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) is a large program designed to systematically investigate the X-ray properties of young stellar/substellar objects in the Taurus star forming region. This paper summarizes selected key findings from XEST.

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