Physics
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008xmm..prop..154d&link_type=abstract
XMM-Newton Proposal ID #06055801
Physics
Stars, White Dwarfs, Solar System, Hd179949
Scientific paper
For 2 contrasting systems we plan to investigate the influence the Hot Jupiters have upon their host stars using phase (planetary orbital and stellar rotational) resolved spectroscopy. By combining our X-ray and UV data with contemporaneous optical spectropolarimetric observations we will be able to test and enhance current models for the magnetic interaction between stars and their giant close-in planets.
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