Dynamic structure of a stellar envelope under the magnetic induction and radiation fields

Details Dynamic structure of a stellar envelope under the magnetic induction and radiation fields Dynamic structure of a stellar envelope under the magnetic induction and radiation fields

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001hell.confe..79m&link_type=abstract

"5th Hellenic Astronomical Conference, held 20-22 September, 2001 in Crete, Greece. Online at http://www.astro.auth.gr/elaset/he

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Scientific paper

In this paper we show a perturbative dinamical analysis of the cool envelope of Be stars under the magnetic induction, radiation and gravitational fields. We consider the magnetohydrostatic model by Ringuelet-Iglesias (RI) as a first order approximation. For small perturbations this method gives a density distribution similar to that obtained by the RI model. When the perturbation is increased, the numerical results show a lower density region at the poles. Nevertheless, we do not obtain a thin disk like other authors.

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