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Table A.2.

Reddening-corrected line intensity ratios, interstellar extinction, diagnostic line ratios, densities, and oxygen abundances for the emission line sources of Haro 14.

Ion L21 L22 L23 L24 L25 L26 L27 L28 L29 L33
4861 Hβ 1.000 1.000 1.000 1.000 1.000 1.000 1.000 1.000 1.000 1.000
4959 [OIII] 0.218±0.013 0.180±0.009 0.536±0.034 0.411±0.026 1.613±0.053 1.360±0.049 0.582±0.035 1.543±0.074 0.430±0.054 0.575±0.073
5007 [OIII] 0.654±0.018 0.555±0.013 1.635±0.070 1.187±0.041 4.820±0.133 4.020±0.119 1.697±0.071 4.625±0.196 1.271±0.090 1.632±0.123
6300 [OI] 0.181±0.010 0.162±0.008 0.531±0.033 0.365±0.017 0.422±0.022 0.232±0.022 0.503±0.032 0.403±0.033 0.501±0.047 0.222±0.041
6363 [OI] 0.068±0.007 0.058±0.006 0.150±0.016 0.129±0.011 0.139±0.013 0.052±0.015 0.169±0.017 0.140±0.020 0.149±0.024 0.094±0.031
6548 [NII] 0.110±0.011 0.134±0.010 0.144±0.027 0.160±0.012 0.151±0.015 0.132±0.018 0.222±0.022 0.162±0.020 0.173±0.029 0.168±0.039
6563 Hα 2.870±0.068 2.870±0.050 2.870±0.165 2.870±0.104 2.870±0.110 2.870±0.118 2.870±0.152 2.870±0.168 2.870±0.229 2.870±0.253
6584 [NII] 0.359±0.015 0.407±0.013 0.437±0.040 0.497±0.023 0.470±0.024 0.438±0.028 0.660±0.041 0.533±0.038 0.548±0.053 0.553±0.066
6678 HeI 0.017±0.005 0.023±0.004 0.026±0.011 0.034±0.011 0.026±0.009 0.046±0.015 0.018±0.017 0.036±0.019 0.021±0.022 0.054±0.029
6717 [SII] 0.669±0.018 0.702±0.013 0.999±0.062 1.052±0.041 0.956±0.040 0.745±0.035 1.176±0.066 0.954±0.059 1.110±0.096 0.857±0.082
6731 [SII] 0.468±0.014 0.484±0.010 0.697±0.045 0.728±0.030 0.667±0.029 0.513±0.026 0.835±0.049 0.646±0.041 0.784±0.070 0.664±0.065
7065 HeI 0.014±0.006 0.015±0.004 0.005±0.008 0.035±0.014 0.034±0.012 0.032±0.016 0.013±0.021 0.022±0.013 0.038±0.021 0.061±0.040
7136 [ArIII] 0.062±0.019 0.054±0.010 0.070±0.031 0.108±0.047 0.126±0.034 0.148±0.047 0.141±0.057 0.139±0.027 0.099±0.067 0.191±0.075
9068 [SIII] 0.107±0.020 0.115±0.014 0.085±0.031 0.104±0.049 0.207±0.040 0.183±0.045 0.128±0.046 0.215±0.035 0.095±0.063 0.170±0.091
FHβ 2.0±0.1 4.2±0.1 1.5±0.3 3.4±0.2 1.8±0.1 1.5±0.1 0.8±0.1 0.6±0.1 1.1±0.2 0.7±0.1
CHβ 0.090±0.020 0.081±0.014 0.398±0.048 0.171±0.030 0.171±0.032 0.164±0.034 0.150±0.044 0.179±0.049 0.244±0.066 0.217±0.073
AV 0.195±0.042 0.176±0.031 0.859±0.103 0.370±0.065 0.369±0.069 0.354±0.074 0.323±0.095 0.386±0.105 0.527±0.143 0.469±0.159
E(B-V) 0.063±0.014 0.057±0.010 0.277±0.033 0.119±0.021 0.119±0.022 0.114±0.024 0.104±0.031 0.124±0.034 0.170±0.046 0.151±0.051
[O III]λ5007/Hβ 0.654±0.032 0.555±0.021 1.635±0.377 1.187±0.101 4.820±0.417 4.020±0.367 1.697±0.196 4.625±0.626 1.271±0.280 1.632±0.371
[O I]λ6300/Hα 0.063±0.004 0.056±0.003 0.185±0.023 0.127±0.008 0.147±0.009 0.081±0.008 0.175±0.014 0.141±0.014 0.175±0.024 0.077±0.016
[N II]λ6584/Hα 0.125±0.006 0.142±0.005 0.152±0.021 0.173±0.010 0.164±0.010 0.153±0.011 0.230±0.017 0.186±0.016 0.191±0.025 0.193±0.029
[S II]λλ6717,6731/Hα 0.396±0.010 0.413±0.008 0.591±0.060 0.620±0.027 0.565±0.026 0.438±0.022 0.701±0.042 0.557±0.039 0.660±0.070 0.530±0.060
Ne (cm−3) < 100 < 100 < 100 < 100 < 100 < 100 < 100 < 100 < 100 ∼100
12+log(O/H)2 8.14 8.18 8.15 8.17 8.21 8.22 8.27 8.26 8.20 8.13

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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