87 citations · 119 across the 4 of their papers we have counts for
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Protodiscs around Hot Magnetic Rotator Stars
M. Maheswaran, J. P. Cassinelli
We develop equations and obtain solutions for the structure and evolution of a protodisc region that is initially formed with no radial motion and super-Keplerian rotation speed wh…
A Magnetic Rotator Wind Disk Model for Be Stars
M. Maheswaran
A Magnetic Rotator Wind-Disk(MRWD) model is considered for the formation of Keplerian disks around Be stars. Material from low latitudes of the stellar surface flows along magnetic…
Magnetic Rotator Winds and Keplerian Disks of Hot Stars
M. Maheswaran
We consider rotating magnetic stars with winds and disks. We establish a theorem that relates the angular velocity of a disk region with no meridional motion to the angular velocit…
A Magnetically Torqued Disk Model for Be Stars
J. P. Cassinelli, J. C. Brown, M. Maheswaran +2
Despite extensive study, the mechanisms by which Be star disks acquire high densities and angular momentum while displaying variability on many time scales are still far from clear…