The rotational evolution of young low mass stars-Reference-Cited by-同舟云学术

The rotational evolution of young low mass stars

Published:2007-05 Issue:S243 Volume:3 Page:231-240
ISSN:1743-9213
Container-title:Proceedings of the International Astronomical Union
language:en
Short-container-title:Proc. IAU

Author:

Bouvier Jérôme

Abstract

AbstractStar-disk interaction is thought to drive the angular momentum evolution of young stars. In this review, I present the latest results obtained on the rotational properties of low mass and very low mass pre-main sequence stars. I discuss the evidence for extremely efficient angular momentum removal over the first few Myr of pre-main sequence evolution and describe recent results that support an accretion-driven braking mechanism. Angular momentum evolution models are presented and their implication for accretion disk lifetimes discussed.

Publisher

Cambridge University Press (CUP)

Subject

Astronomy and Astrophysics,Space and Planetary Science

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