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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