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Table 3.

Properties of the blue-shifted velocity component for all high-excitation and coronal emission lines in the nuclear spectrum of NGC 6552.

Line λlab log(ncrit) Flux FWHM Vpeak Vout
[μm] [eV] cm−3 [%] [km s−1] [km s−1] [km s−1]
(1) (2) (3) (4) (5) (6) (7) (8)
[FeVIII] 5.447 125.0 6.41 0.61 ± 0.04 637 ± 67 −88 ± 19 629 ± 61
[MgVII] 5.503 186.5 6.53 0.77 ± 0.02 786 ± 37 −36 ± 21 704 ± 25
[MgV] 5.610 109.2 6.60 0.67 ± 0.04 661 ± 22 −167 ± 12 728 ± 22
[NeVI] 7.652 126.2 5.80 0.63 ± 0.03 579 ± 20 −151 ± 10 642 ± 22
[ArV] 7.902 59.8 5.20 0.71 ± 0.07 579 ± 61 −175 ± 21 666 ± 51
[ArIII] 8.991 27.6 5.28 0.67 ± 0.03 683 ± 21 −151 ± 11 731 ± 19
[FeVII] 9.527 99.1 5.74 0.75 ± 0.02 980 ± 35 −79 ± 17 911 ± 26
[SIV] 10.51 34.8 4.75 0.70 ± 0.01 742 ± 20 −98 ± 7 727 ± 17
[NeV] 14.32 97.1 4.51 0.66 ± 0.04 606 ± 21 −175 ± 13 689 ± 23
[NeIII] 15.56 41.0 5.32 0.57 ± 0.02 652 ± 23 −117 ± 10 672 ± 19
[OIV] 25.89 54.9 4.00 0.59 ± 0.13 493 ± 102 −165 ± 75 584 ± 25

Notes. Columns describe the: (1) name of each high-excitation and coronal emission line, (2) intrinsic wavelength from lab, (3) ionisation potential, (4) critical density, (5) percentage of flux in the blue-shifted component, (6) FWHM of the blue-shifted component, (7) velocity offset relative to the narrow component, and (8) the outflow maximal velocity. [NeV]24.32 μm line profile is affected by noise and fringes, and [FeVII]7.815 μm by a spike, both of them have been discarded from the characterisation of the blue-shifted velocity component.

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