Changes between Version 11 and Version 12 of CollidingFlows
- Timestamp:
- 06/30/11 14:06:41 (14 years ago)
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CollidingFlows
v11 v12 107 107 108 108 Here we've plotted the cooling time as a function of density and ram pressure (in units of Kelvin/cc) 109 109 110 [[Image(nPCoolingTime.png, width-400)]] 110 111 111 112 We can then calculate the cooling length of the shock [[latex($L_{cool}=T_{cool} v_{shock}$)]] or the cooling length of the thermal instability [[latex($\lambda_{TI}=T_{cool} c_s \approx L_{cool}$)]] since [[latex($c_s \approx v_{shock}$)]] 112 113 Here are plots of the cooling length as well as the thermal instability length scale. 114 113 115 [[Image(nPCoolingLength.png, width=400)]][[Image(nPTILength.png, width=400)]] 114 116 115 117 We can also calculate the free fall time for the condensations 116 118 [[latex($t_{ff}=\sqrt{\frac{3 \pi}{32 G \rho}}$)]] as well as the Jeans length [[latex($\lambda_J= c_s\sqrt{\frac{\pi}{G\rho}}$)]] plotted below 119 117 120 [[Image(nPFreeFallTime.png, width=400)]][[Image(nPJeansLength.png, width=400)]] 118 121 … … 123 126 124 127 Combining these two time scales gives a clump survivability [[latex($\xi=\frac{t_{cc}}{t_{ff}}$)]] 128 125 129 [[Image(nPTICollapsibility.png)]] which peaks at about .1 126 130 127 131 Plotting the same quantity in n vs V space we have 132 128 133 [[Image(nVTICollapsibility.png)]] 129 134 we can see that optimal parameters are somewhere around a density of 20 and a velocity of 16 km/s although we still need clumps to survive for ~ 10 cloud crushing times before collapsing... Of course if the wind turns off then clumps will be able to survive longer and collapse. It might be better therefore to use finite wind durations...