Studying the Interstellar Medium of H II/BCD Galaxies Using IFU Spectroscopy
Figure 4
Spatial distribution of oxygen abundances in the galaxy Tol 2146-391. Left: g-band acquisition image of the galaxy. The rectangle indicates the FoV of covered by our GMOS-IFU observation. Right: spatial distribution. The isocontours display the H emission. The maximum H emission is indicated in the maps by an X symbol. We considered spaxels with signal-to-noise ratio (S/N) 3 in the [OIII] 4363 line. More details in [33].
