XMM-Newton Proposal 02065304

Details XMM-Newton Proposal 02065304 XMM-Newton Proposal 02065304

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..338s&link_type=abstract

XMM-Newton Proposal ID #02065304

Physics

Hd 1237, Hd 20367, Xmm-Newton Proposal 02065304

Scientific paper

We intend to measure the radiation in the X-ray band (especially the emission at energies higher than 1 keV) of four stars known to host giant planets. The X-ray spectra will be used as input in our models to study the effects of high-energy radiation on planet atmospheres. The selected stars have X-ray luminosity similar to that of young solar analogs, and will serve as a first step to test the influence of the high-energy radiation on the early planetary atmospheres analogous to the young stages of the Solar system, and its subsequent evolution.

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