Observability and diagnostics in the X-ray band of shock-cloud interactions in supernova remnants

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Table 1:

Parameters of the simulated shock-cloud interactions.
Run	${\cal M}$ ^a	$\chi$ ^b	w^c	$T_{\rm psh}$ ^d	$\tau _{\rm cc}$ ^e	therm.
			[km s^-1]	[MK]	[10³ yr]	cond.
HYm40c10	40	10	458	3.0	6.75	no
HYm50c10	50	10	574	4.7	5.41	no
HYm60c10	60	10	688	6.7	4.50	no
RCm40c10	40	10	458	3.0	6.75	yes
RCm50c10	50	10	574	4.7	5.41	yes
RCm60c10	60	10	688	6.7	4.50	yes
RCm50c03	50	03	574	4.7	2.96	yes
RCm50c30	50	30	574	4.7	9.37	yes

Notes. ^(a) Shock Mach number. ^(b) Density contrast cloud/ambient medium. ^(c) Velocity of the SNR shock. ^(d) Temperature of the post-shock ambient medium. ^(e) Cloud crushing time (Klein et al. 1994).

Source LaTeX | All tables | In the text

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