The radial abundance gradient of chlorine in the Milky Way
We determine the radial abundance gradient of Cl in the Milky Way from H II regions spectra. For the first time, the Cl/H ratios are computed by simply adding ionic abundances and not using an ionization correction factor (ICF). We use a collection of published very deep spectra of Galactic H II regions. We have recalculated the physical conditions
Esteban, C. et al.
Fecha de publicación:
9
2015