Table 7: Results of the H$\alpha $ photometry of the galaxies and regions analyzed in this work. The H$\alpha $ flux is corrected for both extinction and the contribution of the [N II] emission lines. Last column shows the age of the last starbursting episode derived comparing W(H$\alpha $) with the predictions given by Leitherer et al. (1999) models.

Object
Flux Luminosity $M_{\rm H~II}$ $M_{\star}$ SFR W(H$\alpha $) Age
  (10-13 erg cm-2 s-1) (1040 erg s-1) (106 $M_{\odot}$) (106 $M_{\odot}$) ($M_{\odot}$ yr-1) (Å) (Myr)
HCG 31              
A1 0.137 $\pm$ 0.015 0.452 $\pm$ 0.049 0.067 $\pm$ 0.007 0.64 $\pm$ 0.07 0.036 $\pm$ 0.004 70 $\pm$ 30 6.8 $\pm$ 0.6
B 0.925 $\pm$ 0.078 3.05 $\pm$ 0.26 0.453 $\pm$ 0.038 8.20 $\pm$ 0.69 0.242 $\pm$ 0.020 80 $\pm$ 20 6.5 $\pm$ 0.3
ACb 11.00 $\pm$ 0.70 36.3 $\pm$ 2.3 5.39 $\pm$ 0.34 18.2 $\pm$ 1.2 2.88 $\pm$ 0.18 500 $\pm$ 40 4.9 $\pm$ 0.1
E 0.452 $\pm$ 0.048 1.49 $\pm$ 0.16 0.222 $\pm$ 0.024 2.62 $\pm$ 0.28 0.118 $\pm$ 0.013 180 $\pm$ 30 5.8 $\pm$ 0.2
F1 1.120 $\pm$ 0.070 3.70 $\pm$ 0.23 0.549 $\pm$ 0.034 0.87 $\pm$ 0.05 0.293 $\pm$ 0.018 1200 $\pm$ 100 3.3 $\pm$ 0.2
F2 0.406 $\pm$ 0.024 1.34 $\pm$ 0.08 0.199 $\pm$ 0.011 0.28 $\pm$ 0.02 0.106 $\pm$ 0.006 1100 $\pm$ 100 3.4 $\pm$ 0.2
G 1.95 $\pm$ 0.11 6.43 $\pm$ 0.36 0.955 $\pm$ 0.054 6.99 $\pm$ 0.39 0.511 $\pm$ 0.029 220 $\pm$ 40 5.5 $\pm$ 0.3
H 0.014 $\pm$ 0.004 0.045 $\pm$ 0.013 0.007 $\pm$ 0.002 0.02 $\pm$ 0.01 0.004 $\pm$ 0.001 420 $\pm$ 100 4.8 $\pm$ 0.2

Mkn 1087
4.78 $\pm$ 0.33 70.0 $\pm$ 4.8 10.39 $\pm$ 0.72 129 $\pm$ 9 5.56 $\pm$ 0.38 90 $\pm$ 20 6.2 $\pm$ 0.1
MB 4.48 $\pm$ 0.31 65.6 $\pm$ 4.5 9.74 $\pm$ 0.67 85 $\pm$ 6 5.21 $\pm$ 0.36 150 $\pm$ 20 6.0 $\pm$ 0.1
#1 0.025 $\pm$ 0.007 0.365 $\pm$ 0.097 0.0541 $\pm$ 0.014 0.67 $\pm$ 0.18 0.029 $\pm$ 0.008 100 $\pm$ 30 6.2 $\pm$ 0.2
#7 0.274 $\pm$ 0.015 4.01 $\pm$ 0.22 0.596 $\pm$ 0.033 2.79 $\pm$ 0.15 0.319 $\pm$ 0.017 390 $\pm$ 30 5.2 $\pm$ 0.2
N 0.155 $\pm$ 0.013 2.27 $\pm$ 0.19 0.337 $\pm$ 0.028 3.34 $\pm$ 0.28 0.180 $\pm$ 0.015 80 $\pm$ 20 6.5 $\pm$ 0.3
K 1.58 $\pm$ 0.09 23.1 $\pm$ 1.3 3.44 $\pm$ 0.20 30.1 $\pm$ 1.7 1.84 $\pm$ 0.11 180 $\pm$ 30 5.8 $\pm$ 0.2

Haro 15

4.66 $\pm$ 0.52 41.8 $\pm$ 4.7 6.21 $\pm$ 0.69 77 $\pm$ 9 3.32 $\pm$ 0.37 90 $\pm$ 20 6.3 $\pm$ 0.3
C 3.23 $\pm$ 0.42 29.0 $\pm$ 3.8 4.31 $\pm$ 0.56 53 $\pm$ 7 2.30 $\pm$ 0.30 110 $\pm$ 20 6.2 $\pm$ 0.2
A 1.27 $\pm$ 0.16 11.4 $\pm$ 1.4 1.69 $\pm$ 0.21 6.7 $\pm$ 0.8 0.91 $\pm$ 0.11 360 $\pm$ 50 4.9 $\pm$ 0.2
B 0.05 $\pm$ 0.02 0.50 $\pm$ 0.20 0.07 $\pm$ 0.03 1.8 $\pm$ 0.7 0.04 $\pm$ 0.01 60 $\pm$ 25 7.0 $\pm$ 0.8

Mkn 1199
14.0 $\pm$ 2.1 48.9 $\pm$ 7.3 7.3 $\pm$ 1.1 140 $\pm$ 21 3.9 $\pm$ 0.6 ... ...
MB 13.6 $\pm$ 2.0 47.5 $\pm$ 7.0 7.1 $\pm$ 1.0 84 $\pm$ 12 3.8 $\pm$ 0.6 ... ...
NE 0.259 $\pm$ 0.065 0.90 $\pm$ 0.23 0.13 $\pm$ 0.03 1.67 $\pm$ 0.42 0.07 $\pm$ 0.02 ... ...
A 0.033 $\pm$ 0.010 0.12 $\pm$ 0.03 0.02 $\pm$ 0.01 0.70 $\pm$ 0.21 0.01 $\pm$ 0.00 ... ...
B 0.064 $\pm$ 0.019 0.22 $\pm$ 0.07 0.03 $\pm$ 0.01 1.35 $\pm$ 0.40 0.02 $\pm$ 0.01 ... ...
e 0.057 $\pm$ 0.017 0.20 $\pm$ 0.06 0.03 $\pm$ 0.01 1.20 $\pm$ 0.36 0.02 $\pm$ 0.01 ... ...

Mkn 5
3.00 $\pm$ 0.08 0.582 $\pm$ 0.014 0.081 $\pm$ 0.010 0.300 $\pm$ 0.012 0.046 $\pm$ 0.011 400 $\pm$ 40 4.9 $\pm$ 0.2
A 2.96 $\pm$ 0.08 0.510 $\pm$ 0.013 0.080 $\pm$ 0.010 0.290 $\pm$ 0.011 0.040 $\pm$ 0.010 442 $\pm$ 66 4.8 $\pm$ 0.2
B 0.042 $\pm$ 0.008 0.072 $\pm$ 0.014 0.0011 $\pm$ 0.0002 0.017 $\pm$ 0.002 0.006 $\pm$ 0.001 50 $\pm$ 20 7.2 $\pm$ 0.8

IRAS 08208+2816
3.29 $\pm$ 0.27 142 $\pm$ 12 21.1 $\pm$ 1.7 166 $\pm$ 14 11.3 $\pm$ 0.9 170 $\pm$ 40 5.8 $\pm$ 0.3
#1 0.046 $\pm$ 0.004 1.97 $\pm$ 0.18 0.29 $\pm$ 0.03 1.65 $\pm$ 0.15 0.156 $\pm$ 0.014 270 $\pm$ 50 5.2 $\pm$ 0.2
#2 0.058 $\pm$ 0.004 2.52 $\pm$ 0.18 0.34 $\pm$ 0.03 2.68 $\pm$ 0.19 0.200 $\pm$ 0.014 190 $\pm$ 40 5.6 $\pm$ 0.3
#3 0.219 $\pm$ 0.011 9.46 $\pm$ 0.48 1.41 $\pm$ 0.07 8.5 $\pm$ 0.4 0.75 $\pm$ 0.04 230 $\pm$ 40 5.3 $\pm$ 0.3
#4 0.031 $\pm$ 0.004 1.32 $\pm$ 0.16 0.20 $\pm$ 0.02 1.9 $\pm$ 0.2 0.105 $\pm$ 0.013 130 $\pm$ 40 6.1 $\pm$ 0.3
#5 0.279 $\pm$ 0.021 12.1 $\pm$ 0.9 1.79 $\pm$ 0.13 8.0 $\pm$ 0.6 0.96 $\pm$ 0.07 330 $\pm$ 40 5.0 $\pm$ 0.2
#6(C) 1.29 $\pm$ 0.07 56 $\pm$ 3 8.3 $\pm$ 0.5 35.0 $\pm$ 1.9 4.43 $\pm$ 0.24 350 $\pm$ 50 5.0 $\pm$ 0.1
#7 0.032 $\pm$ 0.005 1.38 $\pm$ 0.21 0.21 $\pm$ 0.03 1.5 $\pm$ 0.2 0.110 $\pm$ 0.016 180 $\pm$ 50 5.7 $\pm$ 0.4
#8 0.170 $\pm$ 0.017 7.35 $\pm$ 0.74 1.09 $\pm$ 0.11 12.5 $\pm$ 1.3 0.58 $\pm$ 0.06 110 $\pm$ 30 6.2 $\pm$ 0.3
#9 0.067 $\pm$ 0.010 2.91 $\pm$ 0.44 0.43 $\pm$ 0.06 5.9 $\pm$ 0.9 0.23 $\pm$ 0.04 90 $\pm$ 20 6.4 $\pm$ 0.4
#10 0.106 $\pm$ 0.012 4.58 $\pm$ 0.52 0.68 $\pm$ 0.08 7.8 $\pm$ 0.9 0.36 $\pm$ 0.04 110 $\pm$ 30 6.2 $\pm$ 0.3

IRAS 08339+6517b

16.0 $\pm$ 0.7 120 $\pm$ 6 14.5 $\pm$ 0.7 226 $\pm$ 10 9.5 $\pm$ 0.5 110 $\pm$ 10 6.0 $\pm$ 0.2
Companion 0.28 $\pm$ 0.03 2.1 $\pm$ 0.4 0.26 $\pm$ 0.03 4.1 $\pm$ 0.5 0.17 $\pm$ 0.02 31 $\pm$ 5 6.7 $\pm$ 0.2

POX 4

15.5 $\pm$ 0.5 38.4 $\pm$ 1.2 5.70 $\pm$ 0.18 9.77 $\pm$ 0.32 3.05 $\pm$ 0.10 910 $\pm$ 5 4.5 $\pm$ 0.1
#3 0.675 $\pm$ 0.027 1.67 $\pm$ 0.07 0.25 $\pm$ 0.01 0.54 $\pm$ 0.02 0.13 $\pm$ 0.01 840 $\pm$ 10 4.6 $\pm$ 0.2
#6 0.380 $\pm$ 0.030 0.94 $\pm$ 0.07 0.14 $\pm$ 0.01 0.24 $\pm$ 0.02 0.07 $\pm$ 0.01 1110 $\pm$ 25 4.0 $\pm$ 0.2
#7 0.033 $\pm$ 0.004 0.08 $\pm$ 0.01 0.01: 0.05 $\pm$ 0.01 0.01: 415 $\pm$ 20 5.0 $\pm$ 0.2
#9-C 11.2 $\pm$ 0.4 27.8 $\pm$ 1.0 4.12 $\pm$ 0.15 7.06 $\pm$ 0.25 2.20 $\pm$ 0.08 1410 $\pm$ 5 3.1 $\pm$ 0.1
#11 0.178 $\pm$ 0.011 0.44 $\pm$ 0.03 0.07: 0.25 $\pm$ 0.02 0.04: 450 $\pm$ 10 5.0 $\pm$ 0.1
Comp 0.127 $\pm$ 0.011 0.31 $\pm$ 0.03 0.05: 0.79 $\pm$ 0.07 0.02: 320 $\pm$ 5 5.2 $\pm$ 0.2

UM 420

0.695 $\pm$ 0.043 46.8 $\pm$ 2.9 6.95 $\pm$ 0.43 13.75 $\pm$ 0.85 3.71 $\pm$ 0.23 980 $\pm$ 60 4.3 $\pm$ 0.2

SBS 0926+606 A

2.52 $\pm$ 0.12 9.43 $\pm$ 0.45 1.40 $\pm$ 0.07 3.59 $\pm$ 0.17 0.75 $\pm$ 0.04 600 $\pm$ 40 4.8 $\pm$ 0.2
A1 1.46 $\pm$ 0.11 5.46 $\pm$ 0.41 0.81 $\pm$ 0.06 2.08 $\pm$ 0.16 0.43 $\pm$ 0.03 670 $\pm$ 50 4.7 $\pm$ 0.2
A2 1.06 $\pm$ 0.09 3.96 $\pm$ 0.34 0.59 $\pm$ 0.05 1.51 $\pm$ 0.13 0.31 $\pm$ 0.03 510 $\pm$ 60 4.9 $\pm$ 0.2
SBS 0926+606 B 0.631 $\pm$ 0.056 2.36 $\pm$ 0.21 0.35 $\pm$ 0.03 4.76 $\pm$ 0.42 0.19 $\pm$ 0.02 130 $\pm$ 20 6.7 $\pm$ 0.3
Bc 0.327 $\pm$ 0.031 1.22 $\pm$ 0.12 0.18 $\pm$ 0.02 2.47 $\pm$ 0.23 0.10 $\pm$ 0.01 220 $\pm$ 40 5.9 $\pm$ 0.3
SBS 0948+532 1.86 $\pm$ 0.07 78.2 $\pm$ 2.9 11.61 $\pm$ 0.44 18.84 $\pm$ 0.71 6.21 $\pm$ 0.23 810 $\pm$ 30 4.6 $\pm$ 0.2
SBS 1054+365 5.87 $\pm$ 0.22 0.450 $\pm$ 0.017 0.067$\pm$0.003 0.23 $\pm$ 0.01 0.036 $\pm$ 0.001 320 $\pm$ 50 5.2 $\pm$ 0.2
C 5.16 $\pm$ 0.15 0.395 $\pm$ 0.011 0.059$\pm$0.002 0.20 $\pm$ 0.01 0.031 $\pm$ 0.001 490 $\pm$ 40 4.9 $\pm$ 0.1
a 1.30 $\pm$ 0.060 0.100 $\pm$ 0.005 0.015$\pm$0.001 0.05: 0.008: 390 $\pm$ 40 5.0 $\pm$ 0.2
b1 0.062 $\pm$ 0.009 0.005 $\pm$ 0.001 ... 0.02: ... 40 $\pm$ 15 9.8 $\pm$ 1.0
b2 0.062 $\pm$ 0.009 0.005 $\pm$ 0.001 ... 0.02: ... 25 $\pm$ 20 11 $\pm$ 2
e 0.734 $\pm$ 0.041 0.056 $\pm$ 0.003 0.008: 0.03: 0.004: 270 $\pm$ 40 5.5 $\pm$ 0.3
SBS 1211+540 0.817 $\pm$ 0.031 0.141 $\pm$ 0.005 0.021 $\pm$ 0.001 0.05: 0.011: 640 $\pm$ 40 4.8 $\pm$ 0.2
C 0.726 $\pm$ 0.026 0.125 $\pm$ 0.004 0.019 $\pm$ 0.001 0.04: 0.010: 730 $\pm$ 50 4.7 $\pm$ 0.2
a 0.610 $\pm$ 0.030 0.105 $\pm$ 0.005 0.016 $\pm$ 0.001 0.04: 0.008: 490 $\pm$ 60 5.0 $\pm$ 0.2

SBS 1319+579
2.40 $\pm$ 0.15 2.38 $\pm$ 0.15 0.354 $\pm$ 0.022 0.78 $\pm$ 0.05 0.189 $\pm$ 0.012 620 $\pm$ 60 4.9 $\pm$ 0.2
A 1.480 $\pm$ 0.008 1.469 $\pm$ 0.008 0.2182 $\pm$ 0.0012 0.28 $\pm$ 0.02 0.117 $\pm$ 0.001 1300 $\pm$ 80 3.6 $\pm$ 0.4
B 0.107 $\pm$ 0.009 0.106 $\pm$ 0.009 0.0158 $\pm$ 0.0013 0.10 $\pm$ 0.01 0.008 $\pm$ 0.001 150 $\pm$ 30 6.5 $\pm$ 0.4
C 0.579 $\pm$ 0.041 0.575 $\pm$ 0.041 0.0854 $\pm$ 0.0060 0.28 $\pm$ 0.02 0.046 $\pm$ 0.003 320 $\pm$ 40 5.3 $\pm$ 0.3
d 0.056 $\pm$ 0.005 0.056 $\pm$ 0.005 0.0083 $\pm$ 0.0008 0.06 $\pm$ 0.01 0.004 120 $\pm$ 30 7.1 $\pm$ 0.5
e 0.024 $\pm$ 0.003 0.024 $\pm$ 0.003 0.0035 $\pm$ 0.0004 0.03 0.002 100 $\pm$ 30 7.3 $\pm$ 0.8
f 0.081 $\pm$ 0.006 0.080 $\pm$ 0.006 0.0119 $\pm$ 0.0008 0.07 0.006 220 $\pm$ 30 5.9 $\pm$ 0.4
g 0.026 $\pm$ 0.003 0.026 $\pm$ 0.003 0.0038 $\pm$ 0.0004 0.04 0.002 90 $\pm$ 30 7.3 $\pm$ 0.9
i 0.010 $\pm$ 0.002 0.010 $\pm$ 0.001 0.0015 $\pm$ 0.0002 0.02 0.001 50 $\pm$ 20 9.1 $\pm$ 1.1

SBS 1415+437
4.78 $\pm$ 0.20 0.495 $\pm$ 0.021 0.0735 $\pm$ 0.0031 0.14 $\pm$ 0.01 0.039 $\pm$ 0.002 900 $\pm$ 60 4.5 $\pm$ 0.2
Main Body 4.66 $\pm$ 0.19 0.482 $\pm$ 0.020 0.0716 $\pm$ 0.0029 0.11 0.038 $\pm$ 0.002 900 $\pm$ 60 4.5 $\pm$ 0.2
C 4.10 $\pm$ 0.16 0.424 $\pm$ 0.017 0.0630 $\pm$ 0.0025 0.10 0.034 $\pm$ 0.001 1250 $\pm$ 60 3.7 $\pm$ 0.3
A 0.465 $\pm$ 0.022 0.048 $\pm$ 0.002 0.0071 $\pm$ 0.0003 0.02 0.004 1100 $\pm$ 60 4.0 $\pm$ 0.3
B 0.121 $\pm$ 0.009 0.013 $\pm$ 0.001 0.0019 $\pm$ 0.0001 0.01 0.001 200 $\pm$ 30 6.1 $\pm$ 0.2
d 0.096 $\pm$ 0.008 0.010 $\pm$ 0.001 0.0015 $\pm$ 0.0001 ... 0.001 550 $\pm$ 50 4.9 $\pm$ 0.2

III Zw 107
5.29 $\pm$ 0.24 40.1 $\pm$ 1.8 5.96 $\pm$ 0.27 73.9 $\pm$ 3.4 3.19 $\pm$ 0.15 160 $\pm$ 30 5.9 $\pm$ 0.3
A 4.22 $\pm$ 0.18 32.0 $\pm$ 1.4 4.75 $\pm$ 0.20 32.5 $\pm$ 1.4 2.54 $\pm$ 0.11 250 $\pm$ 40 5.6 $\pm$ 0.3
B 0.965 $\pm$ 0.046 7.32 $\pm$ 0.35 1.087 $\pm$ 0.052 44.4 $\pm$ 2.1 0.58 $\pm$ 0.03 80 $\pm$ 30 6.5 $\pm$ 0.5
C 0.101 $\pm$ 0.018 0.77 $\pm$ 0.14 0.114 $\pm$ 0.020 5.6 $\pm$ 1.00 0.061 $\pm$ 0.011 40 $\pm$ 20 7.6 $\pm$ 1.4

Tol 9
10.2 $\pm$ 0.7 22.9 $\pm$ 1.6 3.4 $\pm$ 0.2 27.4 $\pm$ 1.9 1.82 $\pm$ 0.13 130 $\pm$ 30 6.0 $\pm$ 0.3
C 8.5 $\pm$ 0.4 19.0 $\pm$ 1.0 2.83 $\pm$ 0.14 40 $\pm$ 2 1.51 $\pm$ 0.08 200 $\pm$ 30 5.8 $\pm$ 0.2
#1 0.027 $\pm$ 0.002 0.061 $\pm$ 0.005 0.0091 $\pm$ 0.0007 0.13 $\pm$ 0.01 0.005 $\pm$ 0.001 110 $\pm$ 30 6.1 $\pm$ 0.2
#2 0.105 $\pm$ 0.006 0.236 $\pm$ 0.013 0.035 $\pm$ 0.002 0.50 $\pm$ 0.03 0.019 $\pm$ 0.001 180 $\pm$ 30 5.8 $\pm$ 0.2
#3 0.031 $\pm$ 0.004 0.070 $\pm$ 0.009 0.0104 $\pm$ 0.0013 0.15 $\pm$ 0.02 0.006 $\pm$ 0.001 110 $\pm$ 40 6.2 $\pm$ 0.2
#4 0.020 $\pm$ 0.003 0.045 $\pm$ 0.008 0.0066 $\pm$ 0.0011 0.09 $\pm$ 0.02 0.004 $\pm$ 0.001 140 $\pm$ 40 6.0 $\pm$ 0.2
#5 0.31 $\pm$ 0.04 0.69 $\pm$ 0.09 0.102 $\pm$ 0.013 1.46 $\pm$ 0.19 0.055 $\pm$ 0.007 120 $\pm$ 40 6.1 $\pm$ 0.3
#6 0.002: 0.003: 0.0005: 0.01: ... 80 $\pm$ 30 6.3 $\pm$ 0.3
Env 0.45 $\pm$ 0.04 1.017 $\pm$ 0.09 0.151 $\pm$ 0.013 ... ... ... ...

Tol 1457-262
11.4 $\pm$ 0.6 63.3 $\pm$ 3.5 9.4 $\pm$ 0.5 41 $\pm$ 2 5.0 $\pm$ 0.3 340 $\pm$ 50 5.1 $\pm$ 0.2

Obj 1
8.33 $\pm$ 0.49 46.2 $\pm$ 2.7 6.9 $\pm$ 0.4 23.4 $\pm$ 1.4 3.7 $\pm$ 0.2 430 $\pm$ 40 4.9 $\pm$ 0.2
#1 0.354 $\pm$ 0.032 1.97 $\pm$ 0.18 0.29 $\pm$ 0.03 2.09 $\pm$ 0.19 0.156 $\pm$ 0.014 190 $\pm$ 30 5.8 $\pm$ 0.3
#2 0.319 $\pm$ 0.028 1.77 $\pm$ 0.16 0.26 $\pm$ 0.02 1.59 $\pm$ 0.14 0.141 $\pm$ 0.012 230 $\pm$ 40 5.4 $\pm$ 0.3
#3(B) 0.854 $\pm$ 0.049 4.74 $\pm$ 0.27 0.70 $\pm$ 0.04 2.60 $\pm$ 0.15 0.38 $\pm$ 0.02 410 $\pm$ 40 5.0 $\pm$ 0.2
#4 0.444 $\pm$ 0.040 2.47 $\pm$ 0.22 0.37 $\pm$ 0.03 1.82 $\pm$ 0.16 0.196 $\pm$ 0.018 290 $\pm$ 40 5.2 $\pm$ 0.3
#5 0.550 $\pm$ 0.043 3.05 $\pm$ 0.24 0.45 $\pm$ 0.04 1.57 $\pm$ 0.12 0.242 $\pm$ 0.019 440 $\pm$ 50 4.9 $\pm$ 0.2
#6(A) 3.20 $\pm$ 0.22 17.8 $\pm$ 1.2 2.64 $\pm$ 0.18 8.1 $\pm$ 0.6 1.4 $\pm$ 0.1 650 $\pm$ 50 4.6 $\pm$ 0.2
#7(C) 0.621 $\pm$ 0.050 3.45 $\pm$ 0.28 0.51 $\pm$ 0.04 1.71 $\pm$ 0.14 0.27 $\pm$ 0.02 320 $\pm$ 40 5.1 $\pm$ 0.2
#8 0.482 $\pm$ 0.039 2.68 $\pm$ 0.22 0.40 $\pm$ 0.03 2.41 $\pm$ 0.19 0.212 $\pm$ 0.017 230 $\pm$ 40 5.4 $\pm$ 0.3

Obj 2
3.10 $\pm$ 0.14 17.21 $\pm$ 0.78 2.56 $\pm$ 0.12 14.4 $\pm$ 0.7 1.37 $\pm$ 0.06 250 $\pm$ 30 5.2 $\pm$ 0.2
#9 0.623 $\pm$ 0.036 3.46 $\pm$ 0.20 0.51 $\pm$ 0.03 3.8 $\pm$ 0.2 0.275 $\pm$ 0.016 180 $\pm$ 30 5.7 $\pm$ 0.2
#10 0.833 $\pm$ 0.042 4.62 $\pm$ 0.23 0.69 $\pm$ 0.03 4.2 $\pm$ 0.2 0.367 $\pm$ 0.019 230 $\pm$ 40 5.4 $\pm$ 0.2
#11 0.339 $\pm$ 0.024 1.88 $\pm$ 0.13 0.28 $\pm$ 0.02 2.60 $\pm$ 0.18 0.149 $\pm$ 0.011 140 $\pm$ 30 6.0 $\pm$ 0.3
#12 0.495 $\pm$ 0.038 2.75 $\pm$ 0.21 0.41 $\pm$ 0.03 2.16 $\pm$ 0.17 0.218 $\pm$ 0.017 270 $\pm$ 40 5.2 $\pm$ 0.2
#13 0.244 $\pm$ 0.022 1.35 $\pm$ 0.12 0.20 $\pm$ 0.02 1.76 $\pm$ 0.16 0.108 $\pm$ 0.010 150 $\pm$ 30 6.0 $\pm$ 0.2
#14 0.204 $\pm$ 0.014 1.13 $\pm$ 0.078 0.168 $\pm$ 0.012 1.32 $\pm$ 0.09 0.090 $\pm$ 0.006 170 $\pm$ 30 5.8 $\pm$ 0.2

#15
0.085 $\pm$ 0.007 0.474 $\pm$ 0.039 0.070 $\pm$ 0.006 0.80 $\pm$ 0.07 0.038 $\pm$ 0.003 90 $\pm$ 20 6.4 $\pm$ 0.4
#16 0.006 $\pm$ 0.002 0.036 $\pm$ 0.010 0.005 $\pm$ 0.002 0.10 $\pm$ 0.03 0.003 $\pm$ 0.001 60 $\pm$ 30 7.0 $\pm$ 1.0

Arp 252
4.48 $\pm$ 0.30 90.3 $\pm$ 6.1 13.4 $\pm$ 0.9 82.3 $\pm$ 4.9 7.2 $\pm$ 0.5 ... ...
ESO 566-8 4.17 $\pm$ 0.28 84.1 $\pm$ 5.6 12.5 $\pm$ 0.8 45.1 $\pm$ 3.0 6.68 $\pm$ 0.45 440 $\pm$ 40 4.9 $\pm$ 0.3
a1 3.82 $\pm$ 0.19 77.0 $\pm$ 3.8 11.4 $\pm$ 0.6 37.2 $\pm$ 1.9 6.12 $\pm$ 0.30 510 $\pm$ 40 4.2 $\pm$ 0.4
a2 0.085 $\pm$ 0.007 1.72 $\pm$ 0.15 0.26 $\pm$ 0.02 0.85 $\pm$ 0.08 0.136 $\pm$ 0.012 460 $\pm$ 50 4.8 $\pm$ 0.6
ESO 566-7 0.312 $\pm$ 0.022 6.3 $\pm$ 0.4 0.93 $\pm$ 0.07 16.8 $\pm$ 1.2 0.50 $\pm$ 0.04 90 $\pm$ 20 6.1 $\pm$ 0.2
b1 0.165 $\pm$ 0.010 3.3 $\pm$ 0.2 0.49 $\pm$ 0.03 8.9 $\pm$ 0.5 0.264 $\pm$ 0.016 130 $\pm$ 20 5.9 $\pm$ 0.2
b2 0.140 $\pm$ 0.011 2.8 $\pm$ 0.2 0.419 $\pm$ 0.033 7.5 $\pm$ 0.6 0.224 $\pm$ 0.018 80 $\pm$ 20 6.2 $\pm$ 0.2
b3 0.008 $\pm$ 0.002 0.17 $\pm$ 0.04 0.025 $\pm$ 0.007 0.44 $\pm$ 0.12 0.013 $\pm$ 0.004 50 $\pm$ 20 6.4 $\pm$ 0.3
c 0.017 $\pm$ 0.003 0.34 $\pm$ 0.06 0.051 $\pm$ 0.009 0.92 $\pm$ 0.16 0.027 $\pm$ 0.005 500 $\pm$ 100 4.5 $\pm$ 0.8
d 0.008 $\pm$ 0.003 0.16 $\pm$ 0.05 0.024 $\pm$ 0.008 0.43 $\pm$ 0.13 0.013 $\pm$ 0.004 50 $\pm$ 20 6.4 $\pm$ 0.3

NGC 5253c
229 $\pm$ 11 4.39 $\pm$ 0.21 0.651 $\pm$ 0.031 2.22 $\pm$ 0.11 0.348 $\pm$ 0.017 450 $\pm$ 5 5.0 $\pm$ 0.1
a HCG 31AC is NGC 1741.
b Values extracted from López-Sánchez et al. (2006).
c Data of the H$\alpha $ flux and W(H$\alpha $) extracted from Meurer et al. (2006).


Source LaTeX | All tables | In the text