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 2.

Properties of the high-velocity ionized outflow.

Name	log $L_{AGN}^{(1)}$ $L_{\mathrm{AGN}}^{(1)}$	$M_{out}^{(2)}$ $M_{\mathrm{out}}^{(2)}$	$n_{e, out}^{(3)}$ $n_{\mathrm{e,out}}^{(3)}$	$R_{out}^{(4)}$ $R_{\mathrm{out}}^{(4)}$	v_out⁽⁵⁾	${\dot{M}}_{out}^{(6)}$ $\dot M_{\mathrm{out}}^{(6)}$	${\dot{E}}_{out}^{(7)}$ $\dot {E}_{\mathrm{out}}^{(7)}$	$E_{out}^{(8)}$ $E_{\mathrm{out}}^{(8)}$	ϵ⁽⁹⁾
	[erg s⁻¹]	[10⁷ M_⊙]	[cm⁻³]	[kpc]	[km s⁻¹]	[M_⊙ yr⁻¹]	[10⁴² erg s⁻¹]	[10⁵⁶ erg]
J1000+1242	45.7	1.9	1230 ± 450	6	850 ± 115	2.9	0.7 ± 0.7	1.5 ± 0.5	4 × 10⁻⁴
J1010+1413	46	5.2	360 ± 100	7	1190 ± 100	9.1	4 ± 2	7.4 ± 2.4	1.2 × 10⁻³
		10		17		6.7	2.2	12.2	6.7 × 10⁻⁴
J1010+0612	45.6	3.7	360 ± 100	7	1123 ± 155	6.2	2.6 ± 2.5	4.9 ± 1.5	2 × 10⁻³
J1100+0846	46	5.3	336 ± 100	9	977 ± 120	6	1.8 ± 2.8	5.2 ± 2.5	5.5 × 10⁻⁴

Notes.⁽¹⁾AGN bolometric luminosity from Harrison et al. (2014). ⁽²⁾Total mass in outflow. ⁽³⁾Outflow electron density estimated from the [SII] doublet ratio. ⁽⁴⁾Outflow radius. ⁽⁵⁾Maximum outflow velocity, v_max, estimated as in Fiore et al. (2017). ⁽⁶⁾Mass outflow rate. ⁽⁷⁾Outflow kinetic power. ⁽⁸⁾Total energy in outflow. ⁽⁹⁾Coupling efficiency, ${\dot{E}}_{out} / L_{AGN}$ $\dot{E}_{\mathrm{out}}/L_{\mathrm{AGN}}$ . The second line for J1010+1413 reports the outflow properties obtained when considering that all the line emission comes from outflowing gas (see text in Sect. 4).

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