High Molecular-gas to Dust Mass Ratios Predicted in Most Quiescent Galaxies (2021)
Attributed to:
Astronomy and Astrophysics at Edinburgh
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/2041-8213/ac399f
Publication URI: http://dx.doi.org/10.3847/2041-8213/ac399f
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal Letters
Issue: 2