Shock triggered star formation rotational vs nonrotatinoal, different mach

We have the following runs:

Krumholz accretion:

Mach = 1.5: non-rotational (case NR), rotation axis along the shock normal (case RA), rotation axis perp to shock normal (case RP). For the rotational cases, K = Omega*tff = 0.1.

Mach = 3.16: non-rotational



Federrath accretion:

Mach = 1.5, 2.5, 3.16 non-rotational

Mach = 1.5, beta = 4 magnetized (field perpendicular to shock normal)



The shock compression phase prior to the formation of the star all look very similar. The initial formation of the star is at about 2 cloud crushing time for Mach = 1.5, 1.6 cloud crushing time for Mach = 3.16. Initially, the cloud with a newly formed star embedded looks like this:

http://www.pas.rochester.edu/~shuleli/tsf_project/initial_formation.png

For Mach = 1.5, different rotation cases at 2 crushing time:

http://www.pas.rochester.edu/~shuleli/tsf_project/2crushingtime.png

For Mach = 1.5, different rotation cases at 2.5 crushing time:

http://www.pas.rochester.edu/~shuleli/tsf_project/25crushingtime.png

For Mach = 1.5, different rotation cases at 3.6 crushing time:

http://www.pas.rochester.edu/~shuleli/tsf_project/36crushingtime.png

Comparison of Star Mass evolution for different rotations:

http://www.pas.rochester.edu/~shuleli/tsf_project/smass.png

Comparison of Accretion Rate for different rotations:

http://www.pas.rochester.edu/~shuleli/tsf_project/accr.png

Comparison of Wind Material Mixing evolution for different rotations:

http://www.pas.rochester.edu/~shuleli/tsf_project/wmixing.png

Movies
case NR:see previous post
case RA:
​http://www.pas.rochester.edu/~shuleli/tsf_project/tsf_rot1.gif
case RP:
​http://www.pas.rochester.edu/~shuleli/tsf_project/tsf_rot2.gif
Mach = 3.16:
​http://www.pas.rochester.edu/~shuleli/tsf_project/mach3.gif
Mach = 1.5, K = 1 (lateral expansion too strong to be contained by the shock):
​http://www.pas.rochester.edu/~shuleli/tsf_project/K1.gif

Comparison of Star Mass evolution for different Mach:

http://www.pas.rochester.edu/~shuleli/tsf_project/smass2.png

Comparison of Accretion Rate for different Mach:

http://www.pas.rochester.edu/~shuleli/tsf_project/accr2.png

Comparison of Wind Material Mixing evolution for different Mach:

http://www.pas.rochester.edu/~shuleli/tsf_project/mixing2.png

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