Energetics of the molecular gas in the H2 luminous radio galaxy 3C 326: Evidence for negative AGN feedback

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Table 7:

MHD shock model parameters, mass flows and cooling times.
$n_{\rm H}$ ^a	$V_{\rm s}$ ^b	Mass flow	$t_{\rm cool}$ ^c	$M_{\rm gas}$
[cm^-3]	[km s^-1]	[ $M_{\odot}$ yr^-1]	[yrs]	[ $M_{\odot}$ ]
10⁴	4	70 100	19 050	$1.3\times 10^9$
10⁴	15	5950	3320	$2.0\times 10^7$
10⁴	34	730	1000	$7.3\times 10^5$
10³	4	41 050	65 000	$2.7\times 10^9$
10³	24	1100	11 500	$1.3\times 10^7$
10³	40	630	5400	$3.4\times 10^6$

Notes. ^(a) Pre-shock density.
^(b) MHD shock velocity.
^(c) Cooling time.

Source LaTeX | All tables | In the text

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