Constraints on the OH-to-H Abundance Ratio in Infrared-bright Galaxies Derived from the Strength of the OH 35 μm Absorption Feature

  1. Stone, M.
  2. Veilleux, S.
  3. González-Alfonso, E.
  4. Spoon, H.
  5. Sturm, E.
Revista:
Astrophysical Journal

ISSN: 1538-4357,  0004-637X

Ano de publicación: 2018

Volume: 853

Número: 2

Tipo: Artigo

DOI: 10.3847/1538-4357/AAA3DF GOOGLE SCHOLAR
Fonte de datos: Scopus