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Stable Keplerian disks TABLE

Cylindrical disks (no grav support height), gamma=1.001

Time increases downwards and the images (click to enlarge) are logarithmic edge-on views of density. Note that to have pressure equilibrium I've set temp_disk=temp_amb/100, whereas in the binary simulation these temperatures are the same. Also, in order to show as as much info about the structure of disks as possible, the color scale limits are not the same for all maps.

TABLE 1

r_soft=r_d/2; r_th=2r_d	r_soft=r_d/2; r_th=8r_d	r_soft=r_d/2; r_th=16r_d	r_soft=r_d/4; r_th=8r_d	r_soft=r_d/8; r_th=2r_d	r_soft=r_d/8; r_th=8r_d	r_soft=r_d/16; r_th=16r_d
same but 2amr →	same but 2 amr →	same but 2 amr →	same but 3 amr →	same →

Flared disks (support height), gamma=1.001

TABLE 2

r_soft=r_d/2; r_th=2r_d	r_soft=r_d/2; r_th=8r_d	r_soft=r_d/2; r_th=16r_d	r_soft=r_d/4; r_th=8r_d	r_soft=r_d/8; r_th=2r_d	r_soft=r_d/8; r_th=8r_d	r_soft=r_d/16; r_th=16r_d

Flared disks (support height), gamma=1.001, temp_d=temp_amb (instead of press_d=press_amb):

TABLE 3

r_soft=r_d/2; r_th=2r_d	r_soft=r_d/2; r_th=8r_d	r_soft=r_d/2; r_th=16r_d	r_soft=r_d/4; r_th=8r_d	r_soft=r_d/8; r_th=2r_d	r_soft=r_d/8; r_th=8r_d	r_soft=r_d/16; r_th=16r_d

Same as table 3 (r_soft=r_d/8; r_th=8r_d) but for a Plummer gravity soft profile, instead of a spline one:

TABLE 4

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f0-iso.png

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f20-isoP.png

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f40-isoP.png

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f60-isoP.png

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f80-isoP.png

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f100-isoP.png

Here's a movie (clock to enlarge) of the run in table 4 but with the same color bar than the corresponding column in table 3.

This is zoomed out. Note that BC are periodic:

Same as table 3 (r_soft=r_d/8; r_th=8r_d) but for gamma=1.667, instead of 1.001:

TABLE 5

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f0-iso.png

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f20-isoG.png

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f40-isoG.png

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f60-isoG.png

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f80-isoG.png

http://www.pas.rochester.edu/~martinhe/2011/disk/soft8-therm8-f100-isoG.png

Posted: 13 years ago (Updated: 13 years ago)
Author: martinhe
Categories: (none)

Comments

1. Jonathan -- 13 years ago

Shoudn't the disks be more flared in the initial conditions for various values of rth/r_d ?

2. martinhe -- 13 years ago

Yes Jonathan, the smaller the value of r_d, the more flared the disks are.

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