XMM-Newton Observations of X-ray Luminous G-type Stellar Coronae

Details XMM-Newton Observations of X-ray Luminous G-type Stellar Coronae XMM-Newton Observations of X-ray Luminous G-type Stellar Coronae

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002hrxs.confe..22s&link_type=abstract

High Resolution X-ray Spectroscopy with XMM-Newton and Chandra, Proceedings of the international workshop held at the Mullard Sp

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We present results obtained from the analysis of XMM-Newton spectra of the Hertzsprung-gap giant 31 Com and of the pre-main-sequence star HD 283572, two G-type stars in very different evolutionary phases, but having similar high X-ray luminosities. We discuss methodological issues related to the data analysis, as well as the results on the inferred properties of the stellar coronae.

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