Chemical distribution of H II regions towards the Galactic anticentre
Context. The study of the radial variations of metallicity across the Galactic disc is a powerful method for understanding the history of star formation and chemical evolution of the Milky Way. Although several studies about gradients have been performed so far, the knowledge of the Galactic antincentre is still poor. Aims: This work aims to
Fernández-Martín, A. et al.
Fecha de publicación:
1
2017