Molecular Gas Heating, Star Formation Rate Relations, and AGN Feedback in Infrared-Luminous Galaxy Mergers (2022)
Attributed to:
Astrophysics at Oxford 2022 -2025
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3390/universe9010003
Publication URI: http://dx.doi.org/10.3390/universe9010003
Type: Journal Article/Review
Parent Publication: Universe
Issue: 1