High-resolution X-ray spectroscopy of T Tauri stars in the Taurus-Auriga complex
A. TelleschiPaul Scherrer Institut, Würenlingen and Villigen, 5232 Villigen PSI, Switzerland e-mail: [email protected]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]M. AudardColumbia Astrophysics Laboratory, Mail code 5247, 550 West 120th Street, New York, NY 10027, USA (Integral Science Data Centre, Ch. d'Ecogia 16, 1290 Versoix, Switzerland & Geneva Observatory, University of Geneva, Ch. des Maillettes 51, 1290 Sauverny, Switzerland.)L. ScelsiDipartimento di Scienze Fisiche ed Astronomiche, Sezione di Astronomia, Università di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy
2007en
ABI
Аннотация
Context.Differences have been reported between the X-ray emission of accreting and non-accreting stars. Some observations have suggested that accretion shocks could be responsible for part of the X-ray emission in classical T Tauri stars (CTTS).
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