Fig. 13
log(N/O) vs. 12 + log(O/H) abundances. The values of the three GH iiRs resolved in HS 2236+1344 are plotted by red points. The black star corresponds with the integrated value of the galaxy. While the small black open dots corresponds with values found by Izotov et al. (2006b) for a large sample of SDSS starburst galaxies and blue dots show data from Izotov et al. (2012) for a sample of XBCDs.
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