Doing physics in star-forming regions with XMM-Newton

Details Doing physics in star-forming regions with XMM-Newton Doing physics in star-forming regions with XMM-Newton

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008an....329..210m&link_type=abstract

Astronomische Nachrichten, Vol.329, Issue 2, p.210

Astronomy and Astrophysics

Astronomy

Stars: Activity, Stars: Magnetic Fields, Stars: Pre-Main Sequence, T Tauri Stars, X-Rays: Stars

Scientific paper

Star-forming regions have been observed in X-rays since the first generation of satellites in the late 70s. They are very rich in magnetically-controlled X-ray phenomena: stellar flares and star-disk interactions in hundreds of T Tauri stars, confined winds in massive stars, etc. More recently, in a few low-mass stars, X-ray evidence has been found for accretion shocks. Even if it is not dominant, when it is found the influence of the circumstellar environment on X-ray emission gives precious clues on the magnetic structure in the vicinity of young stars.

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