MHDdisk

Data Release

"Dependence of the circumstellar disk formation"

3D view of the star-forming cloud, 5000 yr after the protostar formation

The yellow and green contours show an iso-density surface at n = 5e8 [cm^-3] and an identified Keplerian disk, respectively.
The pink and red contours show iso-velocity surfaces with v_r = 1 and 3 [km/s], respectively.
The tubes present the B-field lines connecting to the Keplerian disk.

Alpha	Theta	L = 6000 [au]	L = 400 [au]
0.2	0	web	web
	45	web	web
	90	web	web
0.4	0	web	web
	45	web	web
	90	web	web
0.6	0	web	web
	45	web	web
	90	web	web

If you can use Windows OS, you can open the source GFA files 6000 [au] 400 [au] by a FREE 3D viewer, 3D AVS Player ENG JPN, for viewing and manipulating the data file.