THE PROPELLER REGIME OF DISK ACCRETION TO A RAPIDLY ROTATING MAGNETIZED STAR  

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Disk accretion to a rapidly rotating star. Matter flow in the "propeller" regime for a star rotating at W*=0.5 WK* , full region.
[video] (.avi,  approx. 4.5 MBt) 

 

Disk accretion to a rapidly rotating star. W*=0.5 WK* , small region.
[video] (.avi,  approx. 3.8 MBt) 

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created by O. Toropina, 2000-2004Your comments are welcome
2000-2007, last updated on 29.01.07