The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?

Journal: The Astrophysical Journal Letters

Published: 2021-03-22

DOI: 10.3847/2041-8213/abe7dd

Affiliations: 27

Authors: 32

Go to article
Institutions Share
National Astronomical Observatory of Japan (NAOJ), NINS, Japan 0.15
University of Cologne (UoC), Germany 0.09
Jet Propulsion Laboratory (JPL), United States of America (USA) 0.06
The Graduate University for Advanced Studies (Sokendai), Japan 0.06
Yale University, United States of America (USA) 0.05
The University of Manchester (UoM), United Kingdom (UK) 0.03
Harvard-Smithsonian Center for Astrophysics (CfA), United States of America (USA) 0.03
NSF National Radio Astronomy Observatory (NRAO), United States of America (USA) 0.03
Rice University, United States of America (USA) 0.03
The University of Texas at Austin (UT Austin), United States of America (USA) 0.03
Rutgers, The State University of New Jersey (RU), United States of America (USA) 0.03
Max Planck Institute for Extraterrestrial Physics (MPE), Germany 0.03
East Asian Observatory (EAO), United States of America (USA) 0.03
University of Colorado Boulder (CU-Boulder), United States of America (USA) 0.03
The University of Chicago (UChicago), United States of America (USA) 0.03
University of Florida (UF), United States of America (USA) 0.03
Boston University (BU), United States of America (USA) 0.03
Massachusetts Institute of Technology (MIT), United States of America (USA) 0.03
Otsuma Women's University, Japan 0.03
Tokyo Gakugei University (TGU), Japan 0.03
Heidelberg University (Uni Heidelberg), Germany 0.03
Atacama Large Millimeter/Submillimeter Array (ALMA), Chile 0.03
Catalan Institution for Research and Advanced Studies (ICREA), Spain 0.02
The University of Arizona (Arizona), United States of America (USA) 0.02
Institute for Space Studies of Catalonia (IEEC), Spain 0.02
The University of Tokyo (UTokyo), Japan 0.01

Return