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2DShockedClumpsSNR

v6	v7
33	33	The thermodynamics in the simulation are governed by an ideal EOS, and an adiabatic index of gamma = 5/3. The abundances are taken to be solar ($\mu=1.3$). Other parameters of interest are the clump radius, clump crushing time, sound crossing time (ambient and clump medium to travel a clump radius), wind crossing time (to travel clump radius):
34	34
35		\|\| $R_{clump}$ \|\| $10^16 ~cm$ \|\|
	35	\|\| $R_{clump}$ \|\| $10^{16} ~cm$ \|\|
36	36	\|\| $t_{cc}$ \|\| $5\times 10^8~s$ \|\|
37	37	\|\| $t_{sc}$ (for ambient) \|\| $5\times 10^8~s$ \|\|