Young Stellar Objects: Accretion and Outflow

Details Young Stellar Objects: Accretion and Outflow Young Stellar Objects: Accretion and Outflow

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...4e..29g&link_type=abstract

The Ultraviolet Universe: Stars from Birth to Death, 26th meeting of the IAU, Joint Discussion 4, 16-17 August 2006, Prague, Cze

Astronomy and Astrophysics

Astronomy

Scientific paper

Young stellar objects are an excellent laboratory to study the physics of accretion and outflow. The relevance of ultraviolet astronomy to study the physics of these objects is reviewed in this contribution. Special emphasis is made in the following aspects: 1. The magnetic interaction between the star and the disk produces high energy radiation and particles that heat the inner disk. The spectral output form this region is described and compared with the theoretical predictions. 2. H[2] and CO electronic transitions are observed in the spectra of the T-Tauri stars allowing an analysis of the circumstellar/disk warm material and its interaction with radiation.

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