Electromagnetic signatures of black hole clusters in the center of super-Eddington galaxies

Open Access

Table 3.

Parameters of BHs and their jets.

${\dot{M}}_{input} / {\dot{M}}_{Edd, SMBH}$ $\dot{M}_{\mathrm{input}}/\dot{M}_{\mathrm{Edd,SMBH}}$	r_orb[cm]	v_orb[cm s⁻¹]	${\dot{M}}_{BH} [g s^{- 1}]$ $\dot{M}_{\mathrm{BH}}[\mathrm{g\,s^{-1}}]$	L_j[erg s⁻¹]	ρ_w[g cm⁻³]	z_recoll[cm]	B₀[G]	B(z_recoll)[G]	l_j[cm]
ζ₁	3.75 × 10¹⁴	1.88 × 10⁹	8.4 × 10¹³	7.56 × 10³³	5.28 × 10⁻¹⁴	1.9 × 10⁸	1.78 × 10⁵	1.37 × 10⁵	4.5 × 10¹⁴
ζ₂	10¹⁶	3.64 × 10⁸	1.55 × 10¹⁴	1.39 × 10³⁴	2.35 × 10⁻¹⁵	5.26 × 10⁹	2.56 × 10⁵	7203	4.73 × 10¹⁴
ζ₃	4.44 × 10¹⁷	5.49 × 10⁷	2.05 × 10¹⁴	1.84 × 10³⁴	3.84 × 10⁻¹⁷	1.77 × 10¹¹	2.95 × 10⁵	245	4.34 × 10¹⁴

Notes. Parameters of BHs and their jets that contribute most to the emission (corresponding to those just outside the wind photosphere) for three accretion rates Ṁ_input onto the SMBH ( $ζ_{1} \equiv 10 {\dot{M}}_{Edd}$ $\zeta_1\equiv 10\dot{M}_{\mathrm{Edd}}$ , $ζ_{2} \equiv 10^{2} {\dot{M}}_{Edd}$ $\zeta_2\equiv 10^2\dot{M}_{\mathrm{Edd}}$ , and $ζ_{3} \equiv 10^{3} {\dot{M}}_{Edd}$ $\zeta_3\equiv 10^3\dot{M}_{\mathrm{Edd}}$ ). All parameters are derived.

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