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2DShockedClumpsSNR

v10	v11
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33		The thermodynamics in the simulation are 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~~, clump crushing time, sound crossing time (ambient and clump medium to travel a clump radius), wind crossing time (to travel clump radius~~):
	33	The thermodynamics in the simulation are 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; $t_{wc}$):
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35	35	\|\| $R_{clump}$ \|\| $10^{16} ~cm$ \|\|