On the Maximum Stellar Rotation to form a Black Hole without an Accompanying Luminous Transient

Journal: The Astrophysical Journal Letters

Published: 2020-09-25

DOI: 10.3847/2041-8213/abb818

Affiliations: 9

Authors: 7

Go to article
Institutions Share
University of Copenhagen (UCPH), Denmark 0.36
University of California, Santa Cruz (UCSC), United States of America (USA) 0.25
NASA Astrophysics Science Division (ASD), United States of America (USA) 0.14
Center for Theoretical Physics, PAS, Poland 0.07
National Institute of Astrophysics, Optics and Electronics (INAOE), CONACYT, Mexico 0.04
National Council of Science and Technology (CONACYT), Mexico 0.04
Monash University, Australia 0.04
ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav), Australia 0.04
University of Birmingham (UB), United Kingdom (UK) 0.04

Return

Except where otherwise noted © 2021 Springer Nature Limited. All Rights Reserved.
partner of AGORA, HINARI, OARE, INASP, ORCID, CrossRef and COUNTER