The XMM-Newton extended survey of the Taurus molecular cloud (XEST)
M. GüdelPaul Scherrer Institut, Würenlingen and Villigen, 5232 Villigen PSI, Switzerland e-mail: [email protected]K. R. BriggsPaul Scherrer Institut, Würenlingen and Villigen, 5232 Villigen PSI, Switzerland e-mail: [email protected]K. ArznerPaul Scherrer Institut, Würenlingen and Villigen, 5232 Villigen PSI, Switzerland e-mail: [email protected]M. AudardColumbia Astrophysics Laboratory, Mail Code 5247, 550 West 120th Street, New York, NY 10027, USAJ. BouvierLaboratoire d'Astrophysique de Grenoble, Université Joseph Fourier - CNRS, BP 53, 38041 Grenoble Cedex, FranceEric D. FeigelsonDepartment of Astronomy & Astrophysics, Penn State University, 525 Davey Lab, University Park, PA 16802, USAE. FranciosiniINAF - Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, ItalyAdrian M. GlauserPaul Scherrer Institut, Würenlingen and Villigen, 5232 Villigen PSI, Switzerland e-mail: [email protected]N. GrossoLaboratoire d'Astrophysique de Grenoble, Université Joseph Fourier - CNRS, BP 53, 38041 Grenoble Cedex, FranceG. MicelaINAF - Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, ItalyJean-Louis MoninLaboratoire d'Astrophysique de Grenoble, Université Joseph Fourier - CNRS, BP 53, 38041 Grenoble Cedex, FranceT. MontmerleLaboratoire d'Astrophysique de Grenoble, Université Joseph Fourier - CNRS, BP 53, 38041 Grenoble Cedex, FranceDeborah PadgettSpitzer Science Center, California Institute of Technology, Mail Code 220-6, Pasadena, CA 91125, USAF. PallaINAF - Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi, 5, 50125 Firenze, ItalyI. PillitteriDipartimento di Scienze Fisiche ed Astronomiche, Università di Palermo, Piazza del Parlamento 1, 90134 Palermo, ItalyL. M. RebullSpitzer Science Center, California Institute of Technology, Mail Code 220-6, Pasadena, CA 91125, USAL. ScelsiDipartimento di Scienze Fisiche ed Astronomiche, Università di Palermo, Piazza del Parlamento 1, 90134 Palermo, ItalyBernardo SilvaCentro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150 Porto, PortugalStephen L. SkinnerCASA, 389, University of Colorado, Boulder, CO 80309-0389, USAB. StelzerINAF - Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, ItalyA. TelleschiPaul Scherrer Institut, Würenlingen and Villigen, 5232 Villigen PSI, Switzerland e-mail: [email protected]
2006en
ABI
Annotatsiya
Context.The Taurus Molecular Cloud (TMC) is the nearest large star-forming region, prototypical for the distributed mode of low-mass star formation. Pre-main sequence stars are luminous X-ray sources, probably mostly owing to magnetic energy release.
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