The corona of the very active RS CVn system GT Mus

Details The corona of the very active RS CVn system GT Mus The corona of the very active RS CVn system GT Mus

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop...61m&link_type=abstract

XMM-Newton Proposal ID #05018001

Computer Science

Stars, White Dwarfs, Solar System, Gt Mus, Xmm-Newton Proposal 05018001

Scientific paper

We want to determine the properties of the very active RSCVn system GT Mus. It has been recently detected with IBIS onboard of Integral in the band between 20 and 40 keV making it one of the most extreme active star. The study of the light curve and spectral variations will allow to better understand the nature of the emission of such complex and (likely) interacting system. The RGS spectrum will be used for a detailed analysis of the temperature stratificaton and electronic density.

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