Magnetic Jets from Young Stars: high-angular resolution observations

Details Magnetic Jets from Young Stars: high-angular resolution observations Magnetic Jets from Young Stars: high-angular resolution observations

Nov 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009sf2a.conf....3d&link_type=abstract

SF2A-2009: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, held 29 June - 4 July 2009 in

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Supersonic jets are one of the most spectacular manifestation of the formation of a young star. Although their connection with magnetic processes is well established, the exact origin of jets is still a major open issue in star formation. I review in this contribution constraints on magnetic jet launching models derived from high-angular resolution observations of the inner 100 AUs in T Tauri winds. I then discuss open questions and future directions in jet studies, in particular the expected contributions of near-infrared and radio interferometry (with the second generation VLTI instrumentation and ALMA/NOEMA).

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