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Table 4.

Reddening-corrected line intensity ratios, interstellar extinction, diagnostic line ratios, densities, and oxygen abundances for the high-excitation blobs in Haro 14.

Ion Ex1 Ex2 Ex3 Ex4 Ex5 Ex6 Ex7 Ex8
4861 Hβ 1.000 1.000 1.000 1.000 1.000 1.000 1.000 1.000
4959 [OIII] 1.593 ± 0.048 1.798 ± 0.561 1.291 ± 0.050 1.102 ± 0.018 0.966 ± 0.175 1.055 ± 0.208 1.000 ± 0.017 1.080 ± 0.016
5007 [OIII] 4.799 ± 0.123 5.371 ± 1.610 3.787 ± 0.122 3.281 ± 0.045 3.147 ± 0.444 3.104 ± 0.513 2.981 ± 0.039 3.211 ± 0.038
6300 [OI] 0.405 ± 0.021 0.320 ± 0.219 0.232 ± 0.022 0.037 ± 0.005 0.395 ± 0.104 0.442 ± 0.118 0.042 ± 0.004 0.170 ± 0.006
6363 [OI] 0.145 ± 0.013 0.120 ± 0.150 0.058 ± 0.015 0.012 ± 0.004 0.152 ± 0.067 0.091 ± 0.056 0.013 ± 0.003 0.057 ± 0.004
6548 [NII] 0.154 ± 0.014 0.071 ± 0.089 0.136 ± 0.020 0.069 ± 0.004 0.047 ± 0.055 0.088 ± 0.059 0.067 ± 0.004 0.116 ± 0.006
6563 Hα 2.870 ± 0.101 2.870 ± 1.211 2.870 ± 0.128 2.870 ± 0.054 2.870 ± 0.547 2.870 ± 0.649 2.870 ± 0.048 2.870 ± 0.046
6584 [NII] 0.473 ± 0.023 0.116 ± 0.101 0.432 ± 0.030 0.216 ± 0.006 0.318 ± 0.092 0.365 ± 0.108 0.211 ± 0.006 0.356 ± 0.009
6678 HeI 0.028 ± 0.010 0.043 ± 0.065 0.043 ± 0.016 0.028 ± 0.002 0.135 ± 0.065 0.049 ± 0.030 0.028 ± 0.001 0.028 ± 0.002
6717 [SII] 0.933 ± 0.035 0.263 ± 0.146 0.750 ± 0.038 0.239 ± 0.005 0.711 ± 0.152 0.735 ± 0.176 0.256 ± 0.005 0.610 ± 0.011
6731 [SII] 0.644 ± 0.025 0.156 ± 0.105 0.512 ± 0.028 0.171 ± 0.004 0.396 ± 0.095 0.559 ± 0.137 0.177 ± 0.004 0.427 ± 0.008
7065 HeI 0.023 ± 0.008 0.167 ± 0.113 0.030 ± 0.015 0.021 ± 0.002 0.072 ± 0.041 0.067 ± 0.060 0.019 ± 0.002 0.017 ± 0.003
7136 [ArIII] 0.131 ± 0.030 0.056 ± 0.056 0.158 ± 0.054 0.089 ± 0.005 0.176 ± 0.089 0.122 ± 0.088 0.077 ± 0.003 0.086 ± 0.009
9068 [SIII] 0.221 ± 0.035 0.078 ± 0.093 0.191 ± 0.052 0.208 ± 0.011 0.107 ± 0.089 0.116 ± 0.086 0.182 ± 0.008 0.150 ± 0.014
FHβ 2.5 ± 0.1 0.4 ± 0.6 1.9 ± 0.1 225.2 ± 6.1 0.7 ± 0.5 1.1 ± 1.5 129.6 ± 3.1 9.0 ± 0.2
CHβ 0.104 ± 0.029 0.497 ± 0.351 0.138 ± 0.037 0.113 ± 0.016 0.479 ± 0.159 0.650 ± 0.188 0.101 ± 0.014 0.114 ± 0.013
AV 0.225 ± 0.063 1.074 ± 0.758 0.298 ± 0.080 0.243 ± 0.034 1.036 ± 0.343 1.404 ± 0.407 0.218 ± 0.030 0.245 ± 0.029
E(B − V) 0.072 ± 0.020 0.346 ± 0.245 0.096 ± 0.026 0.078 ± 0.011 0.334 ± 0.111 0.453 ± 0.131 0.070 ± 0.010 0.079 ± 0.009
[O III]λ5007/Hβ 4.799 ± 0.328 5.371 ± 11.767 3.787 ± 0.353 3.281 ± 0.121 3.147 ± 2.977 3.104 ± 5.460 2.981 ± 0.097 3.211 ± 0.103
[O I]λ6300/Hα 0.050 ± 0.005 0.042 ± 0.066 0.020 ± 0.005 0.004 ± 0.001 0.053 ± 0.032 0.032 ± 0.030 0.005 ± 0.001 0.020 ± 0.001
[N II]λ6584/Hα 0.165 ± 0.009 0.040 ± 0.051 0.151 ± 0.012 0.075 ± 0.003 0.111 ± 0.055 0.127 ± 0.096 0.073 ± 0.002 0.124 ± 0.003
[S II]λλ6717,6731/Hα 0.549 ± 0.020 0.146 ± 0.135 0.440 ± 0.023 0.143 ± 0.003 0.386 ± 0.152 0.451 ± 0.281 0.151 ± 0.003 0.361 ± 0.007
Ne (cm−3) < 100 < 100 < 100 < 100 < 100 110 < 100 < 100
12+log(O/H)1 8.22 8.20 8.22 8.22 8.09 8.13 8.20 8.19

Notes. Line intensity ratios are normalized to Hβ; the reddening-corrected Hβ flux is in units of 10−16 erg s−1 cm−2.

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