MOKA3D: An innovative approach to 3D gas kinematic modelling - I. Application to AGN ionised outflows

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Table 4.

Energetic properties of the outflow in the sample.

ID	M_out	E_KIN	L_KIN	ṗ_out	n_e	log L_bol
	10³ M_⊙	10⁵² erg	10⁴⁰ erg ⁻¹	10³³ dyne	cm⁻³	erg s⁻¹
NGC 4945	2.1 ± 1.2	3.8 ± 1.9	19 ± 10	3.1 ± 1.5	110	42.3
Circinus	3.3 ± 1.9	1.2 ± 0.6	3.6 ± 1.8	1.3 ± 0.6	300	42.9
NGC 7282	60 ± 36	29 ± 15	27 ± 13	8.6 ± 4.0	260	44.1

Notes. From left to the right: total kinetic energy (E_KIN), total kinetic luminosity (L_KIN), total momentum rate (ṗ_out), electron density (n_e) and AGN bolometric luminosity (log L_bol) in log scale. The uncertainties are computed via error propagation from Eqs. (12)–(14).

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