XMM-Newton Proposal 02072101

Details XMM-Newton Proposal 02072101 XMM-Newton Proposal 02072101

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..366d&link_type=abstract

XMM-Newton Proposal ID #02072101

Physics

2Re J0241-53, Xmm-Newton Proposal 02072101

Scientific paper

Our main scientific goal is to use the capabilities of XMM/RGS to determine the physical characteristics of the X-ray emission (during quiescent and flaring state) of the visual binary 2RE J0241-53. This binary is a strong and very active X-ray emitter, classified as a member of an association of Post-T-Tauri stars. Its study (in particular in terms of chemical coposition) is important for our understanding of the evolution from the T-Tauri phase, and to explain the origin of the X-ray emission in young stars. A detailed study of any FIP effect can be perfomed since the photospheric composition of the stars is known.

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