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

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Table 5:

Observed and bolometric luminosity of the line emission of molecular and ionized gas (H $\alpha$ ).
	Molecular Gas	Ionized gas	Radio source^a	AGN X-ray^b
$\log{{\cal L}_{\rm obs}}$ ^c	41.9	41.3	44.6	40.6
$\log{{\cal L}_{\rm bol}}$ ^d	42.0	43
$\log{E_{\rm kinetic}}$ ^e	57.5	55.7	59.8
$\log{\rm Mass}$ ^f	9.5	7.3
$\log{\tau_{\rm diss}}$ ^g	8.2^h	7.2ⁱ

Notes. ^(a) Radio luminosity measured at 327 MHz. ^(b) X-ray luminosity of the nuclear point source from Ogle et al. (2010). ^(c) erg s^-1. ^(d) erg s^-1. ^(e) erg. ^(f) $M_{\odot}$ . ^(g) yrs. ^(h) For dissipation through the molecular gas. ⁽ⁱ⁾ Assuming that all of the UV/optical line emission is due to dissipation of kinetic energy.

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