Changes between Version 42 and Version 43 of CollidingFlows

Timestamp:

04/21/12 17:31:17 (13 years ago)

Author:

Jonathan

Comment:

—

CollidingFlows

@@ -38 +38 @@
 
 
-Here are the results from the first round of runs using the old cooling curve
+Here are the results from the first round of runs using the old cooling curve.  Most statistics are from hockey puck region centered over the flow with a 40 pc diameter, and a 20 pc width.  Also the column density looking along the flow direction is showing only contributions from matter inside of this hockey puck.  This avoids confusion in the clumpy runs due to the large number of clumps between the edge of the domain and the interaction region...
+
+Dashed lines are for clumpy flow, smooth lines for uniform flow
 
 [[Image(MassEvolution.png, width=400)]]
@@ -60 +62 @@
 [attachment:DensityHistogram.gif]
 
+The smooth Run is completed out to 30 Myr and the clumpy run should be finished soon.  The plan is then to restart these runs at 10 or 20 Myr but with the flow shut off to see if the lack of kinetic energy injection leads to collapse and star formation...
+
+
 == Modified Cooling Params ==
 
-Next we decided to modify the cooling curve (see 
+We also decided to modify the cooling curve to favor core formation (see 
+
 [blog:johannjc04082012])