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Stellar Coronae with XMM-Newton RGS M. Audard, M. Gudel
 

Summary: Stellar Coronae with XMM-Newton RGS
M. Audard, M. Gudel
Paul Scherrer Institut, Wurenlingen and Villigen,
CH-5232 Villigen PSI, Switzerland,
audard@astro.phys.ethz.ch
R. Mewe, A. J. J. Raassen
Space Research Organization of the Netherlands,
Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
E. Behar
Columbia Astrophysics Laboratory, Columbia University,
550 West 120th Street, New York, NY 10027, USA
Abstract
First results from high-resolution coronal spectro-
scopy with the Re ection Grating Spectrometers on
board the XMM-Newton satellite are reviewed. This
paper is structured in two sections: The rst section
presents results in the context of coronal structure of
active stars, while the second discusses X-ray variabil-
ity in these stars.
1. Introduction

  

Source: Audard, Marc - INTEGRAL Science Data Centre & Observatory of Geneva, Université de Genève
Guedel, Manuel - Institut für Astronomie, Universität Wien

 

Collections: Physics