2015/12/18 by R. Amorín, Ricardo Amorín, C. Muñoz–Tuñón +3 · 5 citations
Physics and Astronomy · #Astrophysics #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Galaxy #Luminosity #Metallicity #Physics #Star formation #Stellar, planetary, and galactic studies #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201526397
published as A&A 588, A23 (2016) · 18 pages, 14 Figures, 4 Tables: Accepted for publication in A&A
arxiv created 2015/12/18 · openalex publication_date 2016/01/22 · arxiv updated 2016/03/16 · openalex created_date 2022/08/31 · openalex updated_date 2026/08/06
Context. Tracing the molecular gas-phase in low-mass star-forming galaxies becomes extremely challenging due to significant UV photo-dissociation of CO molecules in their low-dust, low-metallicity ISM environments.