UNIGE document Doctoral Thesis
previous document  unige:12251  next document
add to browser collection

Anisotropic mass loss and stellar evolution : from Be Stars to Gamma Ray Bursts

Georgy, Cyril
Defense Thèse de doctorat : Univ. Genève, 2010 - Sc. 4252 - 2010/09/24
Abstract The treatment of the rotation in stellar evolution codes had considerably improved the predictive capacity of such codes. One of the effects of rotation is the modification of various surface properties of the star. In particular, the stellar winds, which are spherical without rotation, become ever more anisotropic when rotation progressively increases. It is thus important to account precisely for this effect, to obtain a good estimation of the final angular momentum content of the star, which is decisive for the determination of the final fate of the star. In this thesis, we explore the various effects of such anisotropic winds on stellar evolution.
Keywords Evolution stellaireRotationPerte de masse
URN: urn:nbn:ch:unige-122514
Full text
Thesis (7.4 MB) - public document Free access
(ISO format)
GEORGY, Cyril. Anisotropic mass loss and stellar evolution : from Be Stars to Gamma Ray Bursts. Université de Genève. Thèse, 2010. https://archive-ouverte.unige.ch/unige:12251

393 hits



Deposited on : 2010-11-01

Export document
Format :
Citation style :