Probing the X-ray emission from the low mass CTTS DN Tau

Details Probing the X-ray emission from the low mass CTTS DN Tau Probing the X-ray emission from the low mass CTTS DN Tau

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009xmm..prop...32r&link_type=abstract

XMM-Newton Proposal ID #06511201

Physics

Stars, White Dwarfs, Solar System, Dn Tau

Scientific paper

High resolution X-ray spectroscopy of young stellar objects clearly indicates that in classical T~Tauri stars the physical properties of the cooler X-ray emitting plasma are strongly influenced by accretion and outflow processes. The detailed characteristics apparently depend on stellar parameters like mass and radius; however, especially low mass stars are missing in the the existing X-ray data of young, accreting stars. The proposed observation of DN Tau will extend the current sample into the mass regime of M dwarf precursors and intends to derive a more comprehensive picture of the pre-main sequence evolution of low mass stars.

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