Abstract
Abstract: A review is made of recent magnetohydrodynamic simulations of outflows from accretion disks for different distributions of magnetic field threading the disk. The problem of the opening of a closed field line configuration linking a magnetized star and an accretion disk is also discussed.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
