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2DShockedClumpsSNR

v21	v22
33	33
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35		The thermodynamics in the simulation is governed by an ideal EOS (~~specified by $\gamma~~$). The abundances are taken to be solar ($\mu=1.3$). Other parameters of interest are the clump radius ($R_c$), clump-ambient density contrast ($\chi$), clump crushing time ($t_{cc}=\sqrt{\chi} R_c/v_s$), sound crossing time (ambient and clump medium to travel a clump radius; $t_{sc}$), wind crossing time (to travel clump radius; $t_{wc}$):
	35	The thermodynamics in the simulation is governed by an ideal EOS (with $\gamma=5/3$). The abundances are taken to be solar ($\mu=1.3$). Other parameters of interest are the clump radius ($R_c$), clump-ambient density contrast ($\chi$), clump crushing time ($t_{cc}=\sqrt{\chi} R_c/v_s$), sound crossing time (ambient and clump medium to travel a clump radius; $t_{sc}$), wind crossing time (to travel clump radius; $t_{wc}$):
36	36
37	37	\|\| $R_{c}$ \|\| $10^{16} ~cm$ \|\|