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Table 3.

Ionized and warm molecular outflow properties measured from the broadest component of the [OIII]λ5007 Å, Paα and H2 emission lines.

ID Emission FWHM Vmax rout Orientation Data Reference
line (km s−1) (km s−1) (kpc)
J0232 [OIII] 770 −755 ≤2.8 SDSS a
J1010 [OIII] 1350 −890 ≤1.6 NW VLT/VIMOS & MUSE (*) b
J1100 [OIII] 1780 −1240 0.46 SE HST/STIS c
J1152 [OIII] 360 −480 0.13 NE HST/STIS c
J1356 [OIII] 880 −990 ≤3.1 SW VLT/VIMOS b
J1430 [OIII] 955 −745 0.80 NE VLT/VIMOS d
Paα 1800 −1100 0.55 NE VLT/SINFONI e
J1509 [OIII] 1500 −1100 ≤3 SDSS f
Paα 1800 −1200 0.65 GTC/EMIR f
H2 1500 −750 0.75 GTC/EMIR f

Notes. Columns 3–6 correspond to the emission line’s FWHM, Vmax = −(|Vout|+FWHM/2), projected radius and spatial orientation. Column 7 lists the details of the corresponding data.

(*)

VLT/MUSE (PI: G. Venturi, 0104.B-0476) data retrieved from the ESO Archive Science Portal.

References. (a) Villar-Martín et al. (2014); (b) Harrison et al. (2014); (c) Fischer et al. (2018); (d) Harrison et al. (2015); (e) Ramos Almeida et al. (2017); (f) Ramos Almeida et al. (2019).

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