Disc Dispersal Around Young Stars

Details Disc Dispersal Around Young Stars Disc Dispersal Around Young Stars

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aspc..160..176a&link_type=abstract

Astrophysical Discs - An EC Summer School, Astronomical Society of the Pacific, Conference series Vol #160, Edited by J. A. Sell

Astronomy and Astrophysics

Astrophysics

Scientific paper

Young Solar mass stars accrete material from surrounding circumstellar discs for a period of a few million years, after which the discs are dispersed in a brief, poorly understood epoch. I discuss the observational evidence for disc dispersal, and outline some of the theoretical mechanisms that have been advanced to explain it. The implications of the timing of disc loss for stellar angular momentum regulation are also summarized.

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