Conference
An MHD Model of Be Stars with Disks
Abstract
Abstract
An investigation of the formation and evolution of Be stars show that these stars could have dipolar fossil magnetic fields. This magnetic field should constrain the circumstellar magnetic disk and influence its dynamical features. For studying these effects we refine the alphamodel of accretion disks of Shakura and Sunyaev by incorporating into this model the evolution of large-scale magnetic fields. In the frame of …
Authors
Dudorov AE; Pudritz RE
Volume
175
Pagination
pp. 611-616
Publisher
Cambridge University Press (CUP)
Publication Date
2000
DOI
10.1017/s0252921100056633
Conference proceedings
International Astronomical Union Colloquium
ISSN
0252-9211