The accretion engine in pre Main Sequence stars and its role in the evolution of young planetary disks

Details The accretion engine in pre Main Sequence stars and its role in the evolution of young planetary disks The accretion engine in pre Main Sequence stars and its role in the evolution of young planetary disks

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007uasb.conf....3g&link_type=abstract

UV Astronomy: Stars from Birth to Death. Proceedings of the Joint Discussion n.4 during the IAU general Assembly of 2006. Ana I.

Astronomy and Astrophysics

Astronomy

Uv Astronomy, Pre-Main Sequence Stars, Jets, Winds, Young Planetary Disks

Scientific paper

Young stellar objects are an excellent laboratory to study the physics of accretion and outflow. The impact of this physics on the evolution of the constituents of pre-main sequence systems (star, disk) and the relevance of ultraviolet instrumentation to study this process are outlined. Special emphasis is made on the spectral characterization of the gravito-magnetic engine as well as on the role of the engine on the evolution of the inner disk. A recent review on the relevance of UV instrumentation to make progress in the understanding of star formation can be found in Ǵomez de Castro et al (2006).

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