Stellar Coronae with \textit{XMM-Newton} RGS. I. Coronal Structure

Authors :: Guedel, M.
Audard, M.
Boggende, A. J. den
Brinkman, A. C.
Herder, J. W. den
Kaastra, J. S.
Mewe, R.
Raassen, A. J. J.
de Vries, C.
Behar, E.
Cottam, J.
Kahn, S. M.
Paerels, F. B. S.
Peterson, J. M.
Rasmussen, A. P.
Sako, M.
Branduardi-Raymont, G.
Sakelliou, I.
Erd, C.
Guedel, M.
Audard, M.
Boggende, A. J. den
Brinkman, A. C.
Herder, J. W. den
Kaastra, J. S.
Mewe, R.
Raassen, A. J. J.
de Vries, C.
Behar, E.
Cottam, J.
Kahn, S. M.
Paerels, F. B. S.
Peterson, J. M.
Rasmussen, A. P.
Sako, M.
Branduardi-Raymont, G.
Sakelliou, I.
Erd, C.
Publication Year :: 2000
Abstract: First results from high-resolution coronal spectroscopy with the {\it XMM-Newton} Reflection Grating Spectrometers (RGS) are reviewed. Five stellar systems (HR 1099, Capella, Procyon, YY Gem, AB Dor) have been observed. The emphasis of the present paper is on overall coronal structure. Elemental abundances in {\it active stars} are found to be `anomalous' in the sense that they tend to increase with increasing First Ionization Potential (FIP - i.e., signifying an inverse FIP effect). Coronal densities are measured at levels of a few times $10^{10}$ cm$^{-3}$ for cooler plasma, although there are indications for very high densities in the hotter plasma components.<br />Comment: To appear in Proc. of "X-ray astronomy 2000",(Palermo Sep. 2000), Eds. R. Giacconi, L. Stella, S. Serio, ASP Conf. Series, in press

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