Molecular Gas Properties on Cloud Scales across the Local Star-forming Galaxy Population

Journal: The Astrophysical Journal Letters

Published: 2020-09-18

DOI: 10.3847/2041-8213/abb3be

Affiliations: 28

Authors: 37

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Institutions Share
Heidelberg University (Uni Heidelberg), Germany 0.16
Max Planck Institute for Astronomy (MPIA), Germany 0.15
The Ohio State University (OSU), United States of America (USA) 0.11
Australian National University (ANU), Australia 0.05
Infrared Processing and Analysis Center (IPAC), JPL, United States of America (USA) 0.05
National Geographic Institute (IGN), Spain 0.05
Institut de Radioastronomie Millimétrique (IRAM), France 0.04
Ghent University (UGent), Belgium 0.03
University of Wyoming, United States of America (USA) 0.03
University of Antofagasta, Chile 0.03
University of Maryland, College Park (UMCP), United States of America (USA) 0.03
University of Bonn (Uni Bonn), Germany 0.03
Princeton University, United States of America (USA) 0.03
Max Planck Institute for Extraterrestrial Physics (MPE), Germany 0.03
European Southern Observatory (ESO), Germany 0.03
University of Alberta (U of A), Canada 0.03
Research Institute in Astrophysics and Planetology (IRAP), France 0.03
University of California, San Diego (UC San Diego), United States of America (USA) 0.03
Carnegie Observatories, CIS, United States of America (USA) 0.01
University of Chile, Chile 0.01
IPSL Laboratory for Studies of Radiation and Matter in Astrophysics (LERMA), France 0.01
University of Massachusetts Amherst (UMass Amherst), United States of America (USA) 0.01
Lyon Centre for Astrophysics Research (CRAL), France 0.01
Harvard-Smithsonian Center for Astrophysics (CfA), United States of America (USA) 0.01

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