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Table 1

Photometric properties of the identified star-forming complexes: distances, magnitudes, and sizes.

IRAS Nuclei Complex Number d near d CM M F435 MF435W − MF814W reff  r r Hα
and IP number of knots (kpc) (kpc) (pc) (pc) (pc)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)

04315-0840 1, IV 1 4 4.6 ... −11.37 1.02 38 166 386
2 1 4.2 ... −9.34 0.85 21 93 260
06076-2139 2, III 1 2 11.5 ... −12.86 0.34 77 306 1216
2 2 11.3 ... −12.02 0.21 59 283 902
3 1 12.6 ... −10.53 0.29 53 121 384
4 1 12.3 ... −10.27 0.26 51 116 544
5 1 11.1 ... −10.77 −0.23 41 89 608
6 1 9.9 ... −11.88 0.35 66 137 942
07027-6011 S 2, I-II 1 1 4.6 ... −11.20 0.62 31 127 740
2 1 9.5 ... −10.73 0.07 61 186 670
08355-4944 1, IV 1 2 3.3 ... −12.94 0.26 52 149 705
08572+3915 N 2, III 1 1 6.5 6.8 −12.96 0.20 105 405 1716
08572+3915 SE 2, III 1 5 4.4 6.8 −14.54 0.44 176 636 1514
2 3 9.3 11.2 −14.05 0.39 199 560 1809
3 2 9.3 11.2 −12.10 0.56 76 322 809
4 1 11.0 12.1 −11.83 0.90 191 312 1144
F10038-3338 1, IV 1 8 10.9 ... −14.33 0.67 235 630 1016
2 4 8.3 ... −12.47 0.98 58 414 551
3 2 12.4 ... −11.34 0.76 43 269 603
4 2 13.4 ... −11.72 0.50 88 252 603
12112+0305 2, III 1 3 3.4 3.8 −15.56 1.26 200 887 1721
2 3 9.4 9.6 −15.77 0.56 212 506 1405
3 2 10.4 10.8 −14.82 0.68 200 583 1217
4 1 11.1 11.6 −12.34 0.56 82 288 1405
14348-1447 2, III 1 2 7.8 7.8 −14.26 2.34 280 909 2167
15250+3609 1, IV 1 4 8.8 ... −14.13 1.09 165 627 1176
F18093-5744 N 3, III 1 3 3.9 3.1 −11.91 0.56 48 170 497
2 3 4.8 6.8 −12.06 1.11 46 178 602
3 1 3.8 6.0 −10.11 0.86 20 74 363
F18093-5744 C 3, III 1 1 6.5 4.3 −9.92 0.84 37 78 482
23128-5919 2, III 1 2 6.8 8.3 −12.30 0.87 83 376 1098

16007+3743 3, III R1 1 16.9 17.1 ... ... 828 ... 1151
R2 1 8.9 9.4 ... ... 884 ... 1375
R3 1 9 5.8 ... ... 851 ... 1562

Notes. Column (1): object designation in the IRAS Point and Faint Source catalogues. In case of several pointings taken with VIMOS data, the orientation (N: North, S: South, SE: South-East, C: Center) of the centered nucleus in that pointing is given. Column (2): number of nuclei in the system (1–3) and interaction phase (IP) that the system is undergoing according to the classification scheme defined in Miralles-Caballero et al. (2011), where I-II indicates first approach, III pre-merger and IV merger phases, respectively. Column (3): identified complex. Column (4): number of knots per complex. Column (5): projected distance to the nearest galaxy. Column (6): projected distance to the mass center of the system. Column (7): absolute magnitude, MF435, not corrected for internal extinction. Column (8): derived photometric color of the complex. Column (9): reff of the brightest knot inside the complex. Column (10): equivalent radius, derived using the size of the knots (see text). Column (11): radius of the complex measured on the Hα map.

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