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Home All issues Volume 505 / No 3 (October III 2009) A&A, 505 3 (2009) 1319-1343 Full HTML
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Table 1:

Main characteristics of the sample of ULIRGs. The galaxies are sorted by decreasing nuclear distance.

IRAS Name		 RA(J2000) Dec(J2000) Spectral Class z $D_{\rm {L}}$a ${\log(L_{\rm {IR}})}$b Scale Morphologyc
  (hh:mm:ss) (deg:mm:ss) (Optical)   (Mpc) (L$_{\odot}$) (kpc arcsec-1)  
IRAS 13156+0435 13:18:07.6 +04:18:59.4 H  II/LINER (G) 0.113 525 12.13 2.058 IP at 36.0 kpc
IRAS 13342+3932 13:36:23.3 +39:16:41.9 Sey1 (E) 0.179 866 12.51 3.026 IP at 25.1 kpc
IRAS 18580+6527 18:58:06.3 +65:31:32.2 H  II/Sey2 (G) 0.176 850 12.26 2.986 IP at 15.0 kpc
IRAS 16007+3743 16:02:36.9 +37:34:39.7 LINER (H) 0.185 898 12.11 3.100 IP at 14.2 kpc
IRAS 06268+3509 06:30:12.6 +35:07:51.9 H  II (C)d 0.169 813 12.51e 2.895 IP at 9.1 kpc
IRAS 08572+3915 09:00:25.4 +39:03:54.4 LINER (E)f 0.058 259 12.17 1.130 IP at 6.1 kpc
IRAS 14348-1447 14:37:38.4 -15:00:22.8 LINER (E) 0.083 378 12.39 1.556 IP at 5.5 kpc
Arp 299g 11:28:30.4 +58:34:10.0 H  II/Sey2 (D)h 0.010 43 11.81 0.205 IP at 5.0 kpc
IRAS 13469+5833 13:48:40.3 +58:18:50.0 H  II (I)i 0.158 755 12.31 2.726 IP at 4.5 kpc
IRAS 12112+0305 12:13:42.9 +02:48:29.0 LINER (E) 0.073 330 12.37 1.395 IP at 4.0 kpc
Mrk 463 13:56:02.8 +18:22:17.2 Sey1/Sey2 (F, G)j 0.050 222 11.81 0.984 DN at 3.8 kpc
IRAS 06487+2208 06:51:45.7 +22:04:27.0 H  II (C) 0.144 682 12.57k 2.522 DN at 1.5 kpc
IRAS 11087+5351 11:11:36.4 +53:35:02.0 Sey1 (G) 0.143 677 12.13 2.507 DN at 1.5 kpc
Mrk 273 13:44:42.0 +55:53:12.1 LINER/Sey2 (B, E)l 0.038 167 12.18 0.749 DN at 0.7 kpc
Arp 220 15:34:57.1 +23:30:11.5 LINER (E) 0.018 78 12.20 0.368 DN at 0.4 kpc
IRAS 17208-0014 17:23:21.9 -00:17:00.9 LINER (A)m 0.043 190 12.43 0.844 SN
IRAS 15250+3609 15:26:59.4 +35:58:37.5 LINER (H)n 0.055 245 12.09 1.072 SN
IRAS 12490-1009 12:51:40.7 -10:25:26.1 H  II/LINER (G) 0.101 465 12.07 1.854 SN
IRAS 14060+2919 14:08:18.9 +29:04:46.9 H  II (E) 0.117 545 12.18 2.113 SN
IRAS 09427+1929 09:45:32.4 +19:15:34.9 H  II (H) 0.149 708 12.10 2.600 SN
IRAS 15206+3342 15:22:38.0 +33:31:35.9 H  II (E) 0.124 580 12.27 2.232 SN
Mrk 231 12:56:14.2 +56:52:25.2 Sey1 (E) 0.042 186 12.57 0.832 SN
a For the luminosity distances, the Wright (2006) cosmology calculator has been used.
b $L_{\rm IR} (8{-}1000~\mu$m) was derived following Sanders & Mirabel (1996) ( $L(8{-}1000~\mu {\rm m})=4\pi {D_{\rm L}}^{2}F_{\rm IR}[L_{\odot}]$, with $F_{\rm FIR}=1.26\times 10^{-14}\times(2.58f_{60}+f_{100})[{\rm Wm}^{-2}]$. The quantities f12, f25, f60, and f100 are the IRAS flux densities in Jy at 12, 25, 60 and 100 $\mu$m.). The IRAS fluxes were obtained from the IRAS Faint Galaxy Sample (Moshir et al. 1993, Vizier on line catalogue II/156A).
c IP means interacting pair, DN double nucleus and SN single nucleus. The distances in kpc represent the projected nuclear distance as measured in the F814W HST image.
d (C) Darling & Giovanelli (2006).
e IRAS fluxes obtained from the IRAS point Source Catalogue.
f (E) Kim et al. (1998).
g Arp 299 is the system formed by NGC 3690 (to the east) and IC 694 (to the west).
h (D) García-Marín et al. (2006).
i Veilleux et al. (1999).
j (F) Miller & Goodrich (1990); (G) García-Marín (2007).
k IRAS fluxes obtained from the IRAS point Source Catalogue.
l (B) Colina et al. (1999).
m (A) Arribas & Colina (2003).
n (H) Veilleux et al. (1995).

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