no code implementations • 4 Jan 2021 • J. R. Goicoechea, A. Aguado, S. Cuadrado, O. Roncero, J. Pety, E. Bron, A. Fuente, D. Riquelme, E. Chapillon, C. Herrera, C. A. Duran
We determine their column densities using coupled excitation, radiative transfer as well as chemical formation and destruction models.
Astrophysics of Galaxies
