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Table 3

Physical parameters derived from spectral lines for the intergalactic Hii regions.

ID M g N e E(BV) N2 O3N2 12+log(O/H)
mag cm-3 N2 O3N2

IG_04_main –15.76 327 0.91 –0.39 0.74 8.67 ± 0.18 8.49 ± 0.1
IG_04_tail –15.31 90 0.84 –0.54 1.01 8.58 ± 0.18 8.40 ± 0.14
IG_17_P1 0.70* –0.58 8.56 ± 0.18
IG_51_P3 –14.58 0.33 –0.54 8.58 ± 0.18
IG_85_P6 –14.22 176 0.70* –0.54 8.58 ± 0.18
IG_52_P7 –14.51 176 0.75 –0.65 1.29 8.52 ± 0.18 8.31 ± 0.14

Notes.

(*)

Given that the Hβ emission line was not detected in two cases, the color excess, E(BV), was assumed to be an average of the values derived for the other four spectra.

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