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Table 5.

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

Ion Ex9 Ex10 Ex11 Ex12 Ex13 Ex14 Ex15 Ex16
4861 Hβ 1.000 1.000 1.000 1.000 1.000 1.000 1.000 1.000
4959 [OIII] 0.947 ± 0.212 1.054 ± 0.028 0.835 ± 0.014 0.652 ± 0.022 0.483 ± 0.035 0.748 ± 0.011 0.695 ± 0.012 0.510 ± 0.033
5007 [OIII] 2.989 ± 0.533 3.066 ± 0.059 2.486 ± 0.029 1.947 ± 0.044 1.474 ± 0.065 2.235 ± 0.023 2.070 ± 0.025 1.432 ± 0.057
6300 [OI] 0.363 ± 0.122 0.216 ± 0.011 0.040 ± 0.004 0.479 ± 0.017 0.336 ± 0.029 0.104 ± 0.004 0.117 ± 0.005 0.488 ± 0.028
6363 [OI] 0.205 ± 0.085 0.075 ± 0.008 0.012 ± 0.003 0.157 ± 0.009 0.127 ± 0.020 0.034 ± 0.003 0.039 ± 0.003 0.161 ± 0.015
6548 [NII] 0.135 ± 0.066 0.138 ± 0.009 0.077 ± 0.006 0.176 ± 0.014 0.139 ± 0.019 0.099 ± 0.007 0.124 ± 0.009 0.216 ± 0.019
6563 Hα 2.870 ± 0.695 2.870 ± 0.072 2.870 ± 0.050 2.870 ± 0.082 2.870 ± 0.153 2.870 ± 0.044 2.870 ± 0.052 2.870 ± 0.132
6584 [NII] 0.326 ± 0.104 0.424 ± 0.015 0.239 ± 0.009 0.525 ± 0.022 0.436 ± 0.031 0.309 ± 0.010 0.390 ± 0.013 0.626 ± 0.034
6678 HeI 0.053 ± 0.034 0.035 ± 0.006 0.027 ± 0.001 0.028 ± 0.007 0.035 ± 0.013 0.027 ± 0.001 0.024 ± 0.002 0.026 ± 0.012
6717 [SII] 0.731 ± 0.195 0.781 ± 0.022 0.238 ± 0.005 1.104 ± 0.034 0.873 ± 0.050 0.429 ± 0.009 0.592 ± 0.012 1.169 ± 0.057
6731 [SII] 0.602 ± 0.164 0.550 ± 0.017 0.168 ± 0.004 0.774 ± 0.024 0.605 ± 0.036 0.303 ± 0.007 0.414 ± 0.009 0.826 ± 0.041
7065 HeI 0.046 ± 0.063 0.015 ± 0.008 0.018 ± 0.002 0.021 ± 0.006 0.012 ± 0.013 0.017 ± 0.001 0.015 ± 0.002 0.020 ± 0.011
7136 [ArIII] 0.075 ± 0.051 0.096 ± 0.017 0.086 ± 0.007 0.113 ± 0.041 0.109 ± 0.052 0.080 ± 0.005 0.081 ± 0.015 0.116 ± 0.046
9068 [SIII] 0.125 ± 0.102 0.152 ± 0.025 0.206 ± 0.012 0.115 ± 0.039 0.118 ± 0.063 0.178 ± 0.008 0.149 ± 0.019 0.123 ± 0.051
FHβ 0.3 ± 0.3 1.1 ± 0.0 88.9 ± 2.1 7.5 ± 0.4 1.6 ± 0.1 46.0 ± 1.1 49.7 ± 1.2 2.7 ± 0.2
CHβ 0.413 ± 0.201 0.107 ± 0.021 0.090 ± 0.015 0.165 ± 0.024 0.066 ± 0.044 0.169 ± 0.013 0.090 ± 0.015 0.183 ± 0.038
AV 0.892 ± 0.435 0.231 ± 0.045 0.195 ± 0.032 0.356 ± 0.052 0.143 ± 0.096 0.365 ± 0.027 0.195 ± 0.033 0.396 ± 0.083
E(B − V) 0.288 ± 0.140 0.074 ± 0.015 0.063 ± 0.010 0.115 ± 0.017 0.046 ± 0.031 0.118 ± 0.009 0.063 ± 0.011 0.128 ± 0.027
[O III]λ5007/Hβ 2.989 ± 3.023 3.066 ± 0.151 2.486 ± 0.081 1.947 ± 0.126 1.474 ± 0.143 2.235 ± 0.076 2.070 ± 0.070 1.432 ± 0.157
[O I]λ6300/Hα 0.071 ± 0.044 0.026 ± 0.003 0.004 ± 0.001 0.055 ± 0.004 0.044 ± 0.007 0.012 ± 0.001 0.014 ± 0.001 0.056 ± 0.006
[N II]λ6584/Hα 0.113 ± 0.062 0.148 ± 0.006 0.083 ± 0.003 0.183 ± 0.009 0.152 ± 0.011 0.108 ± 0.004 0.136 ± 0.005 0.218 ± 0.015
[S II]λλ6717,6731/Hα 0.464 ± 0.202 0.464 ± 0.013 0.142 ± 0.003 0.654 ± 0.022 0.515 ± 0.027 0.255 ± 0.006 0.350 ± 0.007 0.695 ± 0.038
Ne (cm−3) 220 < 100 < 100 < 100 < 100 < 100 < 100 < 100
12+log(O/H)2 8.13 8.20 8.25 8.20 8.17 8.21 8.22 8.25

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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