Internal Rotation of AB Doradus

dc.contributor.author	Hiremath, K. M
dc.date.accessioned	2008-07-22T11:45:47Z
dc.date.available	2008-07-22T11:45:47Z
dc.date.issued	2000
dc.identifier.citation	IAU Symposia, Vol. 195, pp. 399 - 400	en
dc.identifier.issn	0074-1809
dc.identifier.uri	http://hdl.handle.net/2248/2823
dc.description.abstract	Using Chandrasekhar's MHD equations, we solve for the steady part of the internal rotation of AB Doradus. We estimate the size of the convective envelope to be ~40% of the radius and the rotation velocity at the base to be not less than 1.42x10/Sup -4 rad/sec. This study also yields the steady part of the toroidal magnetic field which is distributed throughout the convective envelope. We present rotational and toroidal magnetic field profiles in the interior and conjecture on the time-dependent part of the magnetic field.	en
dc.format.extent	201135 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2000IAUS..195..399H	en
dc.subject	Toroidal Magnetic Field	en
dc.subject	Magnetic Field	en
dc.subject	AB Doradus	en
dc.title	Internal Rotation of AB Doradus	en
dc.type	Article	en