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Summary: Stellar Coronae in the Chandra and XMM-Newton Era
ASP Conference Series, Vol. TBD, 2001
F. Favata & J. Drake
XMM-Newton Probes the Solar Past: Coronal
Abundances of Solar Analogs at Di erent Ages
Manuel Gudel, Marc Audard, Anton Sres, Rudolf Wehrli
Paul Scherrer Institut, Wurenlingen & Villigen, CH-5232 Villigen PSI,
Switzerland
Ehud Behar
Columbia Astrophysics Laboratory, Columbia University, 550 West
120th Street, New York, NY 10027, USA
Rolf Mewe, Anton J. J. Raassen
Space Research Organization of the Netherlands (SRON), Sorbonnelaan
2, 3584 CA Utrecht, The Netherlands
Hilary Magee
Mullard Space Science Laboratory, UCL, Holmbury St. Mary, Dorking,
Surrey, RH5 6NT, UK
Abstract. We present an X-ray spectral analysis of four solar analogs
with di erent ages and magnetic activity levels. We nd largely di erent
coronal compositions. The most active stars tend to show an \Inverse
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