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
Stellar Astrophysics Centre (SAC), AU, Denmark 0.17
Sydney Institute for Astronomy (SIfA), USYD, Australia 0.10
Las Cumbres Observatory Global Telescope Network (LCOGT, Inc.), United States of America (USA) 0.10
School of Physics, UNSW Sydney, Australia 0.07
Mt Stromlo Observatory (MSO), RSAA ANU, Australia 0.06
Theoretical AstroPhysics Including Relativity and Cosmology (TAPIR), Caltech, United States of America (USA) 0.06
School of Physics and Astronomy, UB, United Kingdom (UK) 0.04
Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), France 0.03
MIT Department of Physics, United States of America (USA) 0.03
NASA Ames Research Center (ARC), United States of America (USA) 0.03
Department of Astronomy, UC Berkeley, United States of America (USA) 0.03
Max Planck Institute for Solar System Research (MPS), Germany 0.03
Institute for Astronomy (IvS), KU Leuven, Belgium 0.03
MIT Kavli Institute for Astrophysics and Space Research, United States of America (USA) 0.03
UNC Department of Physics and Astronomy, United States of America (USA) 0.03
Jeremiah Horrocks Institute for Mathematics, Physics and Astronomy, UCLan, United Kingdom (UK) 0.03
Department of Astronomy, BU, United States of America (USA) 0.03
Department of Earth Sciences, UH Mānoa, United States of America (USA) 0.03
Astrophysics Group, Keele University, United Kingdom (UK) 0.03
Institute for Astronomy (IfA), UH Mānoa, United States of America (USA) 0.03
DTU National Space Institute (DTU Space), Denmark 0.01
Institute of Theoretical Physics and Astronomy (TFAI), VU, Lithuania 0.01
Department of Physics, UCSB, United States of America (USA) 0.01
Department of Astronomy, BNU, China 0.01

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