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X-rays from T Tauri: a test case for accreting T Tauri stars
2007
Astronomy and Astrophysics
We test models for the generation of X-rays in accreting T Tauri stars (TTS), using X-ray data from the classical TTS T Tau. High-resolution spectroscopy from the Reflection Grating Spectrometers on XMM-Newton is used to infer electron densities, element abundances and the thermal structure of the X-ray source. We also discuss the ultraviolet light curve obtained by the Optical Monitor, and complementary ground-based photometry. A high-resolution image from Chandra constrains contributions from
doi:10.1051/0004-6361:20066318
fatcat:y2zwu6mijbcltgbjzo5mjjfbiq