Feedback and ionized gas outflows in four low-radio power AGN at z ∼ 0.15

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Volume 685 (May 2024)

A&A, 685 (2024) A122

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Table 3.

Properties of the radio jets and the ionized gas involved in the velocity dispersion enhancement perpendicular to the jets.

Name	log L_1.4 GHz⁽¹⁾	P_jet⁽²⁾	P_jet⁽³⁾	$n_{e}^{(4)}$ $n_{\mathrm{e}}^{(4)}$	M_ion⁽⁵⁾	E_ion⁽⁶⁾	t_jet⁽⁷⁾	E_jet⁽⁸⁾
	[W Hz⁻¹]	[10⁴³ erg s⁻¹]	[10⁴³ erg s⁻¹]	[cm⁻³]	[10⁷ M_⊙]	[10⁵⁶ erg]	[Myr]	[10⁵⁶ erg]
J1000+1242	24.2	8.3 $_{- 2}^{+ 2.5}$ $^{+2.5}_{-2}$	7.3	510	7.5 ± 2.4	0.7 ± 0.3	7.5	195
J1010+1413	24	7.1 $_{- 1.5}^{+ 1.8}$ $^{+1.8}_{-1.5}$	4.9	390	9.3 ± 2.5	2.1 ± 0.8	3.6	80
J1010+0612	24.4	9.8 $_{- 2.5}^{+ 3}$ $^{+3}_{-2.5}$	10.9	280	6.1 ± 1.4	1.2 ± 0.5	0.04	1.2
J1100+0846	24.2	8.3 $_{- 2}^{+ 2.5}$ $^{+2.5}_{-2}$	7.3	260	10 ± 2	1.4 ± 0.4	0.1	2.3

Notes.⁽¹⁾Radio luminosity from Jarvis et al. (2019). ⁽²⁾Kinetic power of the jet estimated from its radio luminosity with Eq. (6) from Bîrzan et al. (2008). ⁽³⁾Kinetic power of the jet estimated from its radio luminosity with Eq. (7) from Heckman & Best (2014). ⁽⁴⁾Electron density from the [SII] doublet ratio. ⁽⁵⁾Mass of ionized gas computed with Eq. (3). ⁽⁶⁾Kinetic energy of ionized gas, $E_{i o n} = M_{i o n} σ_{i o n}^{2} / 2$ $E_\mathrm{ion} = M_\mathrm{ion}\sigma_\mathrm{ion}^{2}/2$ . ⁽⁷⁾Jet traveling time. ⁽⁸⁾Total kinetic energy of jet E_jet = P_jett_jet.

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