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Home All issues Volume 507 / No 3 (December I 2009) A&A, 507 3 (2009) 1313-1326 Full HTML
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Table 3:

General properties of the 33 distant starbursts, of their progenitors whether they can be assumed to be reproduced by a major merger, as well as merger parameters adopted after the modelling.

GOODS id 		z morph $_{\rm kin}$1 Mgas $M_{\rm stellar}$ $f_{\rm gas}$ M2/M12 phase3 orbit4 dTmerger5 Tmerger6 Tsfr[Gyr] $f_{\rm gas}$ (prog)7 $M_{\rm stellar}$ (prog)8
J033210.25-274819.5 0.6087 4 6.658e+09 1.95e+10 0.2545 0.38 1 1 0.09723 0.7134 3.398 0.2759 9.47e+09
J033212.39-274353.6 0.4213 1 1.632e+10 4.074e+10 0.286 - 5 - - - 2.366 - -
J033213.06-274204.8 0.4215 3 7.735e+09 1.549e+10 0.3331 0.26 2 1 0.1646 0.6334 3.614 0.3685 7.333e+09
J033214.97-275005.5 0.6665 4 3.413e+10 8.318e+10 0.2909 1 3 2 2.399 4.532 1.752 0.9096 5.302e+09
J033217.62-274257.4 0.6456 4 1.726e+10 2.399e+10 0.4184 0.7 2 2 0.3429 2.062 1.29 0.4828 1.067e+10
J033219.32-274514.0 0.7241 4 5.992e+09 2.455e+10 0.1962 0.55 2 2 0.483 1.527 3.834 0.3214 1.036e+10
J033219.61-274831.0 0.6699 4 7.68e+09 1.862e+10 0.292 0.33 3 3 0.6233 1.016 2.788 0.4525 7.2e+09
J033219.68-275023.6 0.5595 1 2.136e+10 7.586e+10 0.2197 - 5 - - - 3.205 - -
J033220.48-275143.9 0.6778 4 9.086e+09 1.514e+10 0.3751 0.2222 2 3 1.141 8.422 2.492 0.6051 4.783e+09
J033224.60-274428.1 0.5368 4 5.961e+09 1.202e+10 0.3315 0.55 1 2 0.07111 0.6948 2.166 0.3455 5.886e+09
J033225.26-274524.0 0.6647 4 8.436e+09 3.631e+10 0.1885 0.33 3 2 0.9788 1.729 4.826 0.4773 1.169e+10
J033226.23-274222.8 0.6671 3 2.763e+10 5.248e+10 0.3449 0.05 5 - 1- - 2.536 - -
J033227.07-274404.7 0.7381 4 7.932e+09 1.82e+10 0.3036 0.33 2 2 0.5716 1.01 2.758 0.432 7.421e+09
J033228.48-274826.6 0.6685 4 1.907e+10 4.266e+10 0.309 1 3 3 1.403 2.385 1.182 0.6615 1.045e+10
J033230.43-275304.0 0.6453 4 1.91e+10 4.365e+10 0.3044 0.33 3 3 1.373 2.425 1.664 0.6516 1.093e+10
J033230.57-274518.2 0.6798 4 4.778e+10 1.202e+11 0.2844 0.33 1 1 0.6125 4.582 2.044 0.4134 4.928e+10
J033230.78-275455.0 0.6857 1 9.051e+09 4.571e+10 0.1653 - 5 - - - 7.073 - -
J033231.58-274121.6 0.7041 1 8.325e+09 1.259e+10 0.3981 - 5 - - - 1.904 - -
J033232.96-274106.8 0.4681 4 4.517e+09 1.023e+10 0.3062 0.33 4 3 0.4033 0.5699 2.082 0.4182 4.291e+09
J033233.90-274237.9 0.618 4 2.139e+10 4.571e+10 0.3188 1 4 4 3.06 3.66 1.939 0.801 1.061e+10
J033234.04-275009.7 0.7016 3 7.519e+09 1.23e+10 0.3793 1 4 4 0.4955 0.5406 1.914 0.5024 4.932e+09
J033234.12-273953.5 0.6273 4 1.763e+10 5.012e+10 0.2603 1 3 2 2.618 3.388 1.724 0.9644 1.206e+09
J033237.54-274838.9 0.6637 1 2.492e+10 5.012e+10 0.3321 - 5 - - - 1.663 - -
J033238.60-274631.4 0.6206 1 7.71e+09 3.388e+10 0.1854 0.5 1 5 0.0808 1.891 5.651 0.2047 1.654e+10
J033239.04-274132.4 0.7318 4 7.641e+09 1.38e+10 0.3563 1 4 3 1.072 1.218 2.031 0.6324 3.942e+09
J033239.72-275154.7 0.4151 4 9.879e+09 2.042e+10 0.3261 0.33 2 1 0.3866 0.8263 1.891 0.4101 8.936e+09
J033240.04-274418.6 0.522 4 9.991e+09 5.888e+10 0.1451 0.33 3 4 1.381 1.878 3.453 0.5744 1.466e+10
J033241.88-274853.9 0.667 3 8.07e+09 1.862e+10 0.3023 1 4 2 1.213 1.335 2.776 0.6409 4.792e+09
J033244.20-274733.5 0.736 4 3.155e+10 4.169e+10 0.4308 1 3 2 1.498 2.829 0.6172 0.7408 9.49e+09
J033245.11-274724.0 0.4346 3 1.175e+10 6.31e+10 0.157 1 4 2 2.381 2.892 2.781 0.96 1.496e+09
J033248.28-275028.9 0.4446 3 8.076e+09 1.23e+10 0.3963 0.33 4 2 0.5944 0.7874 2.502 0.5398 4.689e+09
J033249.53-274630.0 0.5221 4 5.923e+09 2.188e+10 0.2131 0.46 1 1 0.05323 1.327 3.657 0.2254 1.077e+10
J033250.53-274800.7 0.736 4 5.832e+09 1.023e+10 0.363 0.33 3 3 0.3807 0.6207 1.692 0.4512 4.408e+09

Notes: 1 morpho-kinematics class following Sect. 2 and Neichel et al.: 1: rotating VF and spiral morphology; 4: non-relaxed galaxies for which both kinematics and morphologies are discrepant from a rotating disk; 3: other galaxies showing either a rotating VF (and a peculiar morphology) or a complex VF and a spiral morphology. 2 M2/M1: merger mass ratio for which M1 is the mass of the observed galaxy and M2 the mass of the interloper. 3 Temporal phase: before 1st pass: 1; between 1st and 2nd pass: 2; near nuclei fusion: 3; disk rebuilding: 4; rotating disk: 5. 4 Merger type/orbit: DIR: 1; INC: 2; POL: 3; RET: 4; other/unknown: 5. 5 dTmerger: time (in Gyr) that have been spent by the galaxy in the merger. 6 Tmerger: total duration of the merger (in Gyr). 7  $f_{\rm gas}$ (prog): gas fraction in progenitors. 8  $M_{\rm stellar}$ (prog): average stellar mass of the progenitors.


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