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.
Aldizkaria:
Astrophysical Journal

ISSN: 1538-4357,  0004-637X

Argitalpen urtea: 2018

Alea: 853

Zenbakia: 2

Mota: Artikulua

DOI: 10.3847/1538-4357/AAA3DF GOOGLE SCHOLAR
Datuen iturria: Scopus