Table 1
The sample of local LIRGs.
Galaxy name | IRAS name | vhela | DL | Nuclear | Ref.c | log LIRd | Ref.e | X-ray data |
(km s-1) | (Mpc) | spect. classb | (L⊙) | |||||
|
||||||||
NGC 23 | IRAS F00073+2538 | 4478 | 64.7 | composite | 1 | 11.1 | 9 | Lehmer et al. (2010) |
NGC 1614 | IRAS F04315–0840 | 4778 | 69.1 | composite | 11 | 11.7 | 9 | XMM-Newton (archive) |
NGC 2369 | IRAS F07160–6215 | 3196 | 46.0 | composite | 8 | 11.1 | 9 | XMM-Newton (our data) |
NGC 3110 | IRAS F10015–0614 | 5014 | 72.6 | H II | 11 | 11.3 | 9 | ′′ |
NGC 3256 | IRAS F10257–4339 | 2790 | 40.1 | H II | 5 | 11.7 | 9 | XMM-Newton (archive) |
NGC 3690* | IRAS F11257+5850 | 3057 | 44.0 | Sy2 | 4 | 11.4 | 2 | ′′ |
IC 694* | ′′ | 3098 | 44.6 | LINER | 4 | 11.6 | 2 | ′′ |
ESO320-G030 | IRAS F11506–3851 | 3038 | 43.7 | H II | 8 | 11.2 | 9 | XMM-Newton (our data) |
IC 860 | IRAS F13126+2453 | 3859 | 55.7 | ··· | 1 | 11.1 | 9 | Lehmer et al. (2010) |
MCG−03-34-064 | IRAS F13197–1627 | 5009 | 72.5 | Sy2 | 11 | 11.1 | 10 | XMM-Newton (archive) |
NGC 5135 | IRAS F13229–2934 | 4074 | 58.8 | Sy2 | 11 | 11.3 | 9 | Levenson et al. (2004) |
NGC 5653 | IRAS F14280+3126 | 3513 | 50.7 | H II | 11 | 11.0 | 9 | Lehmer et al. (2010) |
NGC 5734 | IRAS F14423–2039 | 3998 | 57.7 | composite | 8 | 11.0 | 10 | XMM-Newton (our data) |
NGC 5743 | IRAS F14423–2042 | 4121 | 59.5 | H II | 8 | 10.9 | 10 | ′′ |
IC 4518W* | IRAS F14544–4255 | 4720 | 68.2 | Sy2 | 3 | 11.2 | 8 | XMM-Newton (archive) |
Zw049.057 | IRAS F15107+0724 | 3858 | 55.7 | composite | 7 | 11.2 | 9 | Lehmer et al. (2010) |
IC 4686* | IRAS F18093–5744 | 4948 | 71.6 | H II | 11 | 11.0 | 8 | XMM-Newton (our data) |
IC 4687* | ′′ | 5105 | 73.9 | H II | 11 | 11.3 | 8 | ′′ |
IC 4734 | IRAS F18341–5732 | 4623 | 66.8 | H II | 3 | 11.3 | 9 | ′′ |
MCG+04-48-002 | IRAS 20264+2533 | 4199 | 60.6 | H II | 6 | 11.0 | 10 | XMM-Newton (archive) |
NGC 7130 | IRAS F21453–3511 | 4837 | 70.0 | Sy2 | 11 | 11.4 | 9 | Levenson et al. (2005) |
IC 5179 | IRAS F22132–3705 | 3363 | 48.5 | H II | 11 | 11.2 | 9 | XMM-Newton (our data) |
NGC 7469 | IRAS F23007+0836 | 4840 | 70.0 | Sy1 | 1 | 11.6 | 9 | XMM-Newton (archive) |
NGC 7679 | IRAS 23262+0314 | 5162 | 74.7 | Sy1 | 11 | 11.1 | 9 | ′′ |
NGC 7769 | IRAS F23485+1952 | 4158 | 60.0 | composite | 7 | 10.9 | 10 | ′′ |
NGC 7770* | IRAS F23488+1949 | 4128 | 59.6 | H II | 11 | 10.8 | 8 | ′′ |
NGC 7771* | ′′ | 4302 | 62.1 | H II | 1 | 11.3 | 8 | ′′ |
Notes.
Heliocentric velocity from Spitzer spectra (Pereira-Santaella et al. 2010).
Classification of the nuclear activity from optical spectroscopy. Galaxies classified as composite are likely to be a combination of AGN activity and star-formation.
Logarithm of the IR luminosity, L(8–1000 μm), calculated as defined in Sanders & Mirabel (1996).
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