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The Physics of Pre-Main-Sequence Evolution

Published online by Cambridge University Press:  25 September 2002

J. Bouvier ,
J.-P. Zahn  and
F. Palla
F. Palla*
Affiliation:
Osservatorio Astrofisico di Arcetri, Firenze, Italy
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Abstract

The main properties of pre-main-sequence (PMS) evolution are reviewed, withparticular emphasis on the impact of star formation studies. I will firstdiscuss the basic results established by the work of Hayashi, Iben andCameron in the early '60s. The changes introduced by the constraintsset by the previously ignored phase of protostellar evolution will bethen addressed. Evolutionary models including a variety of physical effects(accretion, rotation, magnetic field) are presented. Finally, theapplication of PMS models to reconstruct the star formation historiesof clusters and associations will be addressed.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 3: Star Formation and the Physics of Young Stars: Summer school on Stellar Physics X , 2002 , pp. 111 - 145
Copyright
© EAS, EDP Sciences, 2002

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