Resolving the ISM at the Peak of Cosmic Star Formation with ALMA: The Distribution of CO and Dust Continuum in z ~ 2.5 Submillimeter Galaxies (2018)
Attributed to:
Durham Astronomy Consolidated Grant 2017-2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aacffa
Publication URI: http://dx.doi.org/10.3847/1538-4357/aacffa
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1