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Table 1.

General properties for all the nine LINERs analysed in this work.

# ID RA (2000) Dec (2000) Morphology z Scale i V Re log(Lbol)
(hh mm ss) (dd mm ss) (pc per ″) (deg) (mag) (″) (erg s−1)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
1 NGC 0266 00 49 47.80 +32 16 39.79 SB(rs)ab 0.0155 351 16 11.8
2 NGC 0315 00 57 48.88 +30 21 08.81 E+ 0.0165 370 57 11.6 25.1 43.30
3 NGC 1052 02 41 04.80 −08 15 20.75 E4 0.005 108 70 11.0 21.9 42.77
4 NGC 3226 10 23 27.01 +19 53 54.68 E2 pec 0.0044 86 69 12.9 30.9 42.33
5 NGC 3245 10 27 18.39 +28 30 26.56 SA00(r) 0.0044 90 62 10.8 25.1 42.29
6 NGC 4278 12 20 06.82 +29 16 50.72 E1-2 0.0021 42 16 10.2 31.6 42.53
7 NGC 4438 12 27 45.59 +13 00 31.78 SA(s)0/a pec 0.0002 29 73 10.9 < 42.36
8 NGC 4750 12 50 07.27 +72 52 28.72 (R)SA(rs)ab 0.0054 129 32 12.1 41.51
9 NGC 5055 13 15 49.33 +42 01 45.40 SA(rs)bc 0.0017 40 55 8.6 41.09

Notes. Columns indicate: (2) RA and (3) Dec: coordinates; (4) morphology, (5) redshift and (6) scale based on their distances to the Local Group barycentre, as given by NED; (7) inclination angle and (8) V mag from HyperLeda; (9) effective radius from Cappellari et al. (2011), Veale et al. (2017, NGC 0315) and see C22 for NGC 1052; and (10) bolometric luminosity estimated from González-Martín et al. (2009b), except for NGC 4750, estimated from Younes et al. (2012).

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