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Table A.1.

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

Ion L11 L12 L13 L14 L15 L16 L17 L18 L19 L20
4861 Hβ 1.000 1.000 1.000 1.000 1.000 1.000 1.000 1.000 1.000 1.000
4959 [OIII] 0.354±0.007 0.539±0.010 0.433±0.014 0.230±0.006 0.361±0.006 0.490±0.012 0.216±0.006 0.355±0.017 0.382±0.015 0.455±0.020
5007 [OIII] 1.033±0.012 1.621±0.019 1.271±0.025 0.701±0.010 1.070±0.011 1.450±0.021 0.647±0.009 1.014±0.026 1.184±0.028 1.374±0.038
6300 [OI] 0.075±0.003 0.092±0.004 0.153±0.006 0.062±0.004 0.056±0.003 0.061±0.005 0.090±0.005 0.235±0.010 0.142±0.011 0.448±0.018
6363 [OI] 0.026±0.002 0.031±0.003 0.053±0.004 0.021±0.003 0.016±0.002 0.019±0.003 0.029±0.003 0.081±0.007 0.041±0.007 0.147±0.010
6548 [NII] 0.110±0.006 0.107±0.005 0.157±0.012 0.123±0.005 0.105±0.004 0.100±0.006 0.120±0.005 0.170±0.014 0.111±0.010 0.174±0.017
6563 Hα 2.870±0.041 2.870±0.041 2.870±0.068 2.870±0.040 2.870±0.032 2.870±0.047 2.870±0.035 2.870±0.079 2.870±0.080 2.870±0.097
6584 [NII] 0.342±0.009 0.329±0.008 0.486±0.018 0.374±0.008 0.317±0.006 0.306±0.008 0.358±0.007 0.532±0.022 0.336±0.015 0.533±0.026
6678 HeI 0.024±0.002 0.028±0.002 0.025±0.003 0.021±0.002 0.026±0.002 0.028±0.002 0.021±0.003 0.030±0.005 0.019±0.005 0.031±0.006
6717 [SII] 0.391±0.007 0.414±0.009 0.725±0.019 0.412±0.007 0.405±0.006 0.388±0.008 0.499±0.008 0.921±0.027 0.566±0.018 1.095±0.039
6731 [SII] 0.276±0.005 0.284±0.007 0.509±0.014 0.287±0.005 0.278±0.005 0.267±0.006 0.345±0.006 0.643±0.020 0.405±0.014 0.770±0.028
7065 HeI 0.015±0.002 0.018±0.002 0.015±0.004 0.014±0.002 0.014±0.001 0.014±0.002 0.014±0.003 0.016±0.005 0.015±0.006 0.023±0.006
7136 [ArIII] 0.058±0.004 0.068±0.005 0.094±0.028 0.052±0.004 0.057±0.003 0.072±0.005 0.042±0.006 0.098±0.034 0.056±0.012 0.092±0.038
9068 [SIII] 0.162±0.007 0.180±0.008 0.123±0.029 0.160±0.007 0.155±0.006 0.177±0.008 0.127±0.009 0.100±0.032 0.124±0.016 0.095±0.036
FHβ 7.5±0.2 4.0±0.1 19.2±0.7 5.2±0.1 9.4±0.2 3.2±0.1 7.2±0.1 7.0±0.3 1.5±0.1 5.7±0.4
CHβ 0.246±0.012 0.105±0.012 0.126±0.020 0.199±0.012 0.121±0.009 0.126±0.014 0.180±0.010 0.151±0.023 0.131±0.023 0.225±0.028
AV 0.531±0.026 0.228±0.026 0.272±0.043 0.430±0.025 0.260±0.020 0.272±0.029 0.388±0.022 0.327±0.050 0.283±0.050 0.487±0.061
E(B-V) 0.171±0.008 0.073±0.008 0.088±0.014 0.139±0.008 0.084±0.007 0.088±0.009 0.125±0.007 0.105±0.016 0.091±0.016 0.157±0.020
[O III]λ5007/Hβ 1.033±0.041 1.621±0.046 1.271±0.063 0.701±0.025 1.070±0.025 1.450±0.050 0.647±0.019 1.014±0.063 1.184±0.069 1.374±0.121
[O I]λ6300/Hα 0.026±0.001 0.032±0.002 0.053±0.002 0.021±0.001 0.019±0.001 0.021±0.002 0.031±0.002 0.082±0.004 0.049±0.004 0.156±0.009
[N II]λ6584/Hα 0.119±0.004 0.114±0.003 0.169±0.007 0.130±0.003 0.110±0.002 0.106±0.003 0.125±0.003 0.185±0.009 0.117±0.006 0.186±0.012
[S II]λλ6717,6731/Hα 0.232±0.005 0.243±0.005 0.430±0.012 0.244±0.005 0.238±0.003 0.228±0.005 0.294±0.005 0.545±0.018 0.338±0.011 0.650±0.029
Ne (cm−3) < 100 < 100 < 100 < 100 < 100 < 100 < 100 < 100 < 100 < 100
12+log(O/H)2 8.26 8.24 8.25 8.27 8.23 8.23 8.22 8.22 8.17 8.20

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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