Changes between Version 11 and Version 12 of CollidingFlows


Ignore:
Timestamp:
06/30/11 14:06:41 (14 years ago)
Author:
Jonathan
Comment:

Legend:

Unmodified
Added
Removed
Modified
  • CollidingFlows

    v11 v12  
    107107
    108108Here we've plotted the cooling time as a function of density and ram pressure (in units of Kelvin/cc)
     109
    109110[[Image(nPCoolingTime.png, width-400)]]
    110111
    111112We 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($c_s \approx v_{shock}$)]]
    112113Here are plots of the cooling length as well as the thermal instability length scale.
     114
    113115[[Image(nPCoolingLength.png, width=400)]][[Image(nPTILength.png, width=400)]]
    114116
    115117We can also calculate the free fall time for the condensations
    116118[[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
    117120[[Image(nPFreeFallTime.png, width=400)]][[Image(nPJeansLength.png, width=400)]]
    118121
     
    123126
    124127Combining these two time scales gives a clump survivability [[latex($\xi=\frac{t_{cc}}{t_{ff}}$)]]
     128
    125129[[Image(nPTICollapsibility.png)]] which peaks at about .1
    126130
    127131Plotting the same quantity in n vs V space we have
     132
    128133[[Image(nVTICollapsibility.png)]]
    129134we 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...