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Table 7:

Keplerian mass ( $M_{\rm Kep}$), dynamical mass ( $M_{\rm dyn}$), neutral gas mass ( $M_{\rm H~I}$), ionized gas mass ( $M_{\rm H~II}$), warm dust mass ( $M_{\rm dust}$), mass of the ionizing star cluster ($M_{\star }$), total stellar mass ( $M_{\rm stars}$), and baryonic mass ( $M_{\rm bar}$) of the galaxies analyzed in this work.

Galaxy 		$M_{\rm Kep}$ $M_{\rm dyn}$ $M_{\rm H~I}$ $M_{\rm H~II}$ $M_{\rm dust}$ $M_{\star }$ $M_{\rm stars}$ $M_{\rm bar}$
  [108 $M_{\odot }$] [108 $M_{\odot }$] [108 $M_{\odot }$] [106 $M_{\odot }$] [106 $M_{\odot }$] [106 $M_{\odot }$] [108 $M_{\odot }$] [108 $M_{\odot }$]
HCG 31 ... ... 74.6 7.8 $\pm$ 0.5 2.56 37.8 $\pm$ 2.8 33.8 141
'' AC 340 850 36.4 5.4 $\pm$ 0.3 ... 18.2 $\pm$ 1.2 14.4 62.5
'' B 26 54 19.4 0.45 $\pm$ 0.04 ... 8.2 $\pm$ 0.7 8.0 33.6
'' E ... 13a ... 0.22 $\pm$ 0.02 ... 2.6 $\pm$ 0.3 0.47 ...
'' F 3.0 15 6.13 0.75 $\pm$ 0.04 ... 0.40 $\pm$ 0.03 0.39 8.5
'' G 21 68 19.4 0.96 $\pm$ 0.05 ... 7.0 $\pm$ 0.4 10.5 36.1
Mkn 1087 560 1800 156 10.4 $\pm$ 9.7 7.8 129 $\pm$ 9 288 494
'' N 2.2 45a ... 0.337 $\pm$ 0.028 ... 3.34 $\pm$ 0.28 4.0 ...
Haro 15 121 365 55 $\pm$ 18 6.2 $\pm$ 0.7 2.1 77 $\pm$ 9 99.2 172
Mkn 1199 82 1650 12.2 7.3 $\pm$ 1.1 3.1 140 $\pm$ 21 275 291
'' NE 2.9 70a ... 0.13 $\pm$ 0.03 ... 1.7 $\pm$ 0.4 17.4 ...
Mkn 5 21 36 0.72 $\pm$ 0.09 0.081 $\pm$ 0.010 0.099 0.300 $\pm$ 0.012 1.5 2.5
IRAS 08208+2816 39 600a ... 21.1 $\pm$ 1.7 8.84 166 $\pm$ 14 298 ...
IRAS 08339+6517 100 370 53 $\pm$ 6 14.5 $\pm$ 0.7 3.91 226 $\pm$ 10 476 546
'' Comp 80 100 7.0 $\pm$ 0.9 0.26 $\pm$ 0.03 ... 4.1 $\pm$ 0.5 18.6 27.9
POX 4 5.0 76 21 5.70 $\pm$ 0.18 0.093 9.8 $\pm$ 0.3 14.3 29.1
'' Comp ... ... ... 0.05 ... 0.79 $\pm$ 0.07 0.88 ...
UM 420 21 200a ... 6.9 $\pm$ 0.4 5.0b 13.8 $\pm$ 0.9 45.6 ...
SBS 0926+606 ... ... 17.7 $\pm$ 7.2 1.75 $\pm$ 0.10 0.37 8.4 $\pm$ 0.6 7.59 30.9
'' A ... 23 9.6 $\pm$ 3.6 1.40 $\pm$ 0.07 ... 3.59 $\pm$ 0.17 2.9 15.5
'' B ... 45 8.1 $\pm$ 3.6 0.35 $\pm$ 0.03 ... 4.8 $\pm$ 0.4 4.7 15.4
SBS 0948+532 21 90a ... 11.6 $\pm$ 0.4 ... 18.8 $\pm$ 0.7 12.6 ...
SBS 1054+365 0.78 15 0.61 $\pm$ 0.06 0.067 $\pm$ 0.003 0.012 0.23 $\pm$ 0.01 0.33 1.13
SBS 1211+540 1.13 1.14 0.24 $\pm$ 0.04 0.021 $\pm$ 0.001 ... 0.05 0.102 0.420
SBS 1319+579 86 140 16.4 0.35 $\pm$ 0.02 0.30 0.78 $\pm$ 0.05 22.9 44.5
SBS 1415+437 2.5 4.9 0.96 $\pm$ 0.07 0.074 $\pm$ 0.003 ... 0.14 $\pm$ 0.01 0.46 1.74
III Zw 107 8.2 180 67 $\pm$ 12 6.0 $\pm$ 0.3 1.25 74 $\pm$ 3 61.8 150
Tol 9 12 580 22 $\pm$ 2 3.4 $\pm$ 0.2 2.41 27.4 $\pm$ 1.9 44.4 106
Tol 1457-262 ... 950 47 9.4 $\pm$ 0.5 1.83 41 $\pm$ 2 87.2 149
'' Obj 1 62 290a ... 6.9 $\pm$ 0.4 ... 23.4 $\pm$ 1.5 46.9 ...
'' Obj 2 ... 150a ... 2.56 $\pm$ 0.12 ... 14.4 $\pm$ 0.7 36.2 ...
Arp 252 ... ... ... 13.4 $\pm$ 0.9 6.32 82.3 $\pm$ 4.9 338 ...
'' ESO 566-8 73 440a ... 12.5 $\pm$ 0.8 ... 45 $\pm$ 3 250 ...
'' ESO 566-7 4 150a ... 0.93 $\pm$ 0.07 ... 16.8 $\pm$ 1.2 88 ...
NGC 5253 ... 83 1.59 $\pm$ 0.09 0.65 $\pm$ 0.03 0.042 2.22 $\pm$ 0.11 11.4 13.5

Notes. (a) Tentative value of $M_{\rm dyn}$ computed using Eqs. (25)-(28) and (29).
(b) The warm dust mass is very probably overestimated because of the FIR contribution by the foreground galaxy UGC 01809.


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