X-rays from jet-driving protostars and T Tauri stars
M. GüdelPaul Scherrer Institut, Würenlingen and Villigen, 5232 Villigen PSI, Switzerland e-mail: [email protected]A. TelleschiPaul 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, USAStephen L. SkinnerCASA, 389, University of Colorado, Boulder, CO 80309-0389, USAK. R. BriggsPaul Scherrer Institut, Würenlingen and Villigen, 5232 Villigen PSI, Switzerland e-mail: [email protected]F. PallaOsservatorio Astrofisico di Arcetri, Largo Enrico Fermi, 5, 50125 Firenze, ItalyC. DougadosLaboratoire d'Astrophysique de Grenoble, Université Joseph Fourier - CNRS, BP 53, 38041 Grenoble Cedex, France
2006en
ABI
Annotatsiya
Aims.We study jet-driving protostars and T Tau stars to characterize their X-ray emission. We seek soft spectral components that may be due to shock emission, and search for soft, shock-induced emission displaced from the stellar position.
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