Paper:	Differential Rotation in Early-Type Stars
Volume:	361, Active OB-Stars: Laboratories For Stellar and Circumstellar Physics
Page:	542
Authors:	Zorec, J.; Fremat, Y.; Domiciano de Souza, A.
Abstract:	Using 2D models of rotating stars, the interferometric measurements of α Eri and its fundamental parameters corrected for gravitational darkening effects we infer that the star might have a core rotating 2.7 times faster than the surface. We explore the consequences on spectral lines produced by surface differential rotation combined with the effects due to a kind of internal differential rotation with rotational energies higher than allowed for rigid rotation which induce geometrical deformations that do not distinguish strongly from those carried by the rigid rotation.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.061 seconds