Changes between Version 4 and Version 5 of TriggeredStarFormation


Ignore:
Timestamp:
01/07/14 18:10:34 (11 years ago)
Author:
Shule Li
Comment:

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  • TriggeredStarFormation

    v4 v5  
    1818||R2|| 1.5 || Perpendicular || 0.1 ||
    1919Simulation lasts till about $4t_{cc}$, which is about 1 million years. The wind should be turned off before that, so we are really looking at an extreme case where the wind lasts for unusually long time. [[BR]]
    20 The following figure shows the at 0.6 million years. [[BR]][[BR]]
     20The following figure shows the at 0.6 million years. (a) non-rotation Mach 1.5(case N), (b) non-rotation Mach 3.16(case N'), (c) parallel rotation Mach 1.5(case R1), (d) perpendicular rotation Mach 1.5(case R2).[[BR]][[BR]]
    2121[[BR]][[BR]]
    22 [[Image(fig2.png,50%)]]
     22[[Image(fig2.png,60%)]]
    2323[[BR]][[BR]]
    2424Movies:[[BR]]
    … …  
    4444
    4545We can study important physics quantities by line plots. The first set of line plots are 1. star mass formed by triggering, 2. accretion rate, 3. mixing ratio of the wind material onto the star, 4. bounded mass (basically the mass of the disk for the rotation cases. for the non-rotating cases, the bounded material evaporates very fast after stage I. [[BR]]
    46 [[Image(fig4.png,50%)]]
     46[[Image(fig4.png,60%)]]
    4747[[BR]][[BR]]
    4848