Very regular high-frequency pulsation modes in young intermediate-mass stars

Journal: Nature

Published: 2020-05-13

DOI: 10.1038/s41586-020-2226-8

Affiliations: 24

Authors: 36

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Institutions Share
Aarhus University (AU), Denmark 0.17
The University of Sydney (USYD), Australia 0.10
Las Cumbres Observatory Global Telescope Network (LCOGT, Inc.), United States of America (USA) 0.10
University of New South Wales (UNSW Sydney), Australia 0.07
Mt Stromlo Observatory (MSO), RSAA ANU, Australia 0.06
California Institute of Technology (Caltech), United States of America (USA) 0.06
Massachusetts Institute of Technology (MIT), United States of America (USA) 0.06
University of Hawai'i at Manoa (UH Mānoa), United States of America (USA) 0.06
University of Birmingham (UB), United Kingdom (UK) 0.04
Keele University, United Kingdom (UK) 0.03
Boston University (BU), United States of America (USA) 0.03
University of Central Lancashire (UCLan), United Kingdom (UK) 0.03
The University of North Carolina at Chapel Hill (UNC), United States of America (USA) 0.03
Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), France 0.03
Science, Engineering and Technology Group (SET), KU Leuven, Belgium 0.03
Max Planck Institute for Solar System Research (MPS), Germany 0.03
University of California, Berkeley (UC Berkeley), United States of America (USA) 0.03
NASA Ames Research Center (ARC), United States of America (USA) 0.03
Technical University of Denmark (DTU), Denmark 0.01
Vilnius University (VU), Lithuania 0.01
University of California, Santa Barbara (UCSB), United States of America (USA) 0.01
Beijing Normal University (BNU), China 0.01

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