Unexplored outflows in nearby low luminosity AGNs - The case of NGC 1052

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Table 3.

Summary of measurements for the second component from MUSE and MEGARA.

Line	σ	ΔV	BPT

	(km s⁻¹)	(km s⁻¹)
Hβ	313 (316) ± 128	637 ± 59	–
[O III]	267 (277) ± 44	582 ± 12	0.52 (0.53) ± 0.14

[O I]	637 (704) ± 167	371 ± 51	−0.07 (−0.07) ± 0.18
Hα-[N II]	281 (277) ± 105	569 ± 12	0.14 (0.14) ± 0.08
[S II]	260 (256) ± 96	571 ± 14	0.16 (0.11) ± 0.14
Hα-[N II]	–	–	0.05 (0.05) ± 0.09
[S II]	445 (434) ± 106	430 ± 175	0.28 (0.28) ± 0.09

Notes. The same as Table 2, but for the secondary component. For the MEGARA data, the [S II] and Hα-[N II] lines were fixed to have the same kinematics (Sect. 3.3.1); we do not report measurements for [O I], due to its low S/N.

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