Accretion-driven X-rays from low-mass classical T Tauri stars

Details Accretion-driven X-rays from low-mass classical T Tauri stars Accretion-driven X-rays from low-mass classical T Tauri stars

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop..169m&link_type=abstract

XMM-Newton Proposal ID #05556501

Physics

Stars, White Dwarfs, Solar System, Vv Sco, Xmm-Newton Proposal Id #05556501

Scientific paper

We propose to obtain a good quality high-resolution X-ray spectrum for the M-type classical T~Tauri star (CTTS) VV~Sco. Our goal is to investigate the characteristics of the X-ray emitting plasma in a star-disk system with a very low mass accreting star. The proposed XMM observation will allow us to test different scenarios proposed to explain accretion-driven X-rays in pre-main-sequence stars, and hence to improve our understanding of the mechanisms and physical conditions which regulate the accretion process in CTTSs and its possible influence on the coronal emission.

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