High- z [OI] emission lines: COLDSIM simulations and ALMA observations
Year: 2025
Type: article
Abstract: Neutral-oxygen [OI] far-infrared emission lines at 63 μm and 145 μm are powerful probes of the physical conditions in the interstellar medium, although they have not been fully exploited in high-redshift studies.
Source: Astronomy and Astrophysics
Institutions: Trieste Astronomical Observatory, Institute for Fundamental Physics of the Universe, National Institute for Astrophysics, University of Trieste, Consejo Nacional de Investigaciones Científicas y Técnicas, Universidad Nacional de Córdoba, Instituto de Astronomía Teórica y Experimental, University of Ljubljana, Astronomical Observatory of Rome, European Southern Observatory, European Southern Observatory, Winona State University, Fondazione ICSC Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $1,865
OpenAlex ID: W4416583746