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Angular momentum evolution of young stars

Published online by Cambridge University Press:  07 August 2014

S. P. Littlefair
S. P. Littlefair*
Affiliation:
Dept. of Physics & Astronomy, University of Sheffield, Sheffield, S6 2NE, UK email: s.littlefair@shef.ac.uk
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Abstract

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In recent years, rotation periods for large numbers of pre-main-sequence stars have become available, covering a wide range of ages and star forming environments. Simultaneously, theoretical developments in the physics of the star-disc interaction have been carried out, and observational measurements of the magnetic field geometry of both fully convective, and pre-main-sequence stars have become available. This review discusses these recent developments, and the extent to which the observational data fits within the existing theoretical frameworks.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S302: Magnetic Fields throughout Stellar Evolution , August 2013 , pp. 91 - 99
Copyright
Copyright © International Astronomical Union 2014 

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