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Home All issues Volume 659 (March 2022) A&A, 659 (2022) A102 Full HTML
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Table 1.

Volume limited sample of local LIRGs.

Object α δ z DL i log LIR Morf. Spectral Ref.
Galaxy name IRAS name J2000.0 J2000.0 class
[h m s] [° ′ ″] [Mpc] [°] [L⊙]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
ESO 297-G011 F01341-3735 N 01 36 23.40 −37 19 17.6 0.0168 73.4 38 ± 11 11.13 1 HII 1,2
NGC 1614 F04315-0840 04 33 59.85 −08 34 44.0 0.0159 69.7 48 ± 2 11.61 2 composite 3
NGC 2369 F07160-6215 07 16 37.73 −62 20 37.4 0.0111 49.7 66 ± 6 11.18 0 composite 4
NGC 3110 F10015-0614 10 04 02.11 −06 28 29.2 0.0163 79.8 57 ± 3 11.37 0 HII 2,3
NGC 3256 F10257-4339 10 27 51.27 −43 54 13.5 0.0093 45.7 − 11.72 2 HII 5
ESO 320-G030 F11506-3851 11 53 11.72 −39 07 48.9 0.0102 52.2 56 ± 4 11.36 0 HII 4,6
MCG-02-33-098 W F12596-1529 13 02 20.00 −15 46 03.7 0.0156 75.2 54 ± 6 11.19 1 composite 2
MCG-02-33-098 E F12596-1529 13 02 20.38 −15 45 59.7 0.0159 75.2 39 ± 1 11.11 1 HII 2,3,7
NGC 5135 F13229-2934 13 25 44.06 −29 50 01.2 0.0136 64.8 53 ± 9 11.33 0 Sy2 1,2,3,9,10
IC 4518 W F14544-4255 14 57 41.18 −43 07 55.6 0.0160 74.6 50 ± 4 11.16 1 Sy2 2,8
IC 4518 E F14544-4255 14 57 44.46 −43 07 52.9 0.0154 71.2 75 ± 2 11.12 1 − 4
... F17138-1017 17 16 35.79 −10 20 39.4 0.0172 76.7 50 ± 1 11.39 2 composite/HII 2
IC 4734 F18341-5732 18 38 25.70 −57 29 25.6 0.0154 68.5 58 ± 10 11.28 0 HII 2
NGC 7130 F21453-3511 21 48 19.52 −34 57 04.5 0.0160 67.6 50 ± 9 11.33 2 Sy2 3,8,9,10
IC 5179 F22132-3705 22 16 09.10 −36 50 37.4 0.0112 46.7 62 ± 5 11.13 0 HII 3,7
NGC 7469 F23007+0836 23 03 15.62 +08 52 26.4 0.0160 66.7 39 ± 5 11.54 1 Sy1 8,9,10,11

Notes. Column (1): Galaxy name. Column (2): IRAS denomination from Sanders et al. (2003). Columns (3) and (4): Right ascension (hours, minutes, seconds) and declination (degrees, arcminutes, arcseconds), respectively, from the NASA Extragalactic Database (NED). Column (5): Redshift. Column (6): Luminosity distance from NED. Column (7): Inclination. Column (8): Infrared luminosity (LIR(8–1000) μm) calculated from the IRAS flux densities f12, f25, f60, and f100 (Sanders et al. 2003). Column (9): Morphological class (0 identifies isolated objects, 1 pre − coalescence systems, and 2 merger objects). Column (10): Nuclear activity class (HII = HII region-like, Sy2 = Seyfert 2 y Sy1 = Seyfert 1, composite).

References. Nuclear classification: 1: Kewley et al. (2001); 2: Corbett et al. (2003); 3:Yuan et al. (2010); 4:Pereira-Santaella et al. (2011); 5: Lípari et al. (2000); 6: van den Broek et al. (1991); 7: Veilleux et al. (1995); 8: Pereira-Santaella et al. (2010); 9: Alonso-Herrero et al. (2012); 10: Alonso-Herrero et al. (2009); 11: Petric et al. (2011).

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