Changes between Version 2 and Version 3 of TriggeredStarFormation
- Timestamp:
- 01/07/14 18:07:46 (11 years ago)
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TriggeredStarFormation
v2 v3 20 20 The following figure shows the at 0.6 million years. [[BR]][[BR]] 21 21 [[BR]][[BR]] 22 [[Image(fig2.png )]]22 [[Image(fig2.png,40%)]] 23 23 [[BR]][[BR]] 24 24 Movies:[[BR]] … … 44 44 45 45 We 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 )]]46 [[Image(fig4.png,40%)]] 47 47 [[BR]][[BR]] 48 48 … … 85 85 86 86 87