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A radio-detected type Ia supernova with helium-rich circumstellar material.

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Title: A radio-detected type Ia supernova with helium-rich circumstellar material.
Authors: Kool EC; The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, Stockholm, Sweden. erik.kool@astro.su.se., Johansson J; The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, Stockholm, Sweden.; The Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm, Sweden., Sollerman J; The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, Stockholm, Sweden., Moldón J; Instituto de Astrofísica de Andalucía, Consejo Superior de Investigaciones Científicas (CSIC), Granada, Spain.; Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester, UK., Moriya TJ; National Astronomical Observatory of Japan, National Institutes of Natural Sciences, Mitaka, Japan.; School of Physics and Astronomy, Faculty of Science, Monash University, Clayton, Victoria, Australia., Mattila S; Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Turku, Finland.; School of Sciences, European University Cyprus, Nicosia, Cyprus., Schulze S; The Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm, Sweden., Chomiuk L; Center for Data Intensive and Time Domain Astronomy, Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA., Pérez-Torres M; Instituto de Astrofísica de Andalucía, Consejo Superior de Investigaciones Científicas (CSIC), Granada, Spain.; Facultad de Ciencias, Universidad de Zaragoza, Zaragoza, Spain., Harris C; Center for Data Intensive and Time Domain Astronomy, Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA., Lundqvist P; The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, Stockholm, Sweden., Graham M; Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA., Yang S; The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, Stockholm, Sweden.; Henan Academy of Sciences, Zhengzhou, China., Perley DA; Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK., Strotjohann NL; Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel., Fremling C; Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA., Gal-Yam A; Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel., Lezmy J; Univ. Lyon, Univ. Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, France., Maguire K; School of Physics, Trinity College Dublin, The University of Dublin, Dublin, Ireland., Omand C; The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, Stockholm, Sweden., Smith M; Univ. Lyon, Univ. Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, France.; School of Physics and Astronomy, University of Southampton, Southampton, UK., Andreoni I; Joint Space-Science Institute, University of Maryland, College Park, MD, USA.; Department of Astronomy, University of Maryland, College Park, MD, USA.; Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA., Bellm EC; DIRAC Institute, Department of Astronomy, University of Washington, Seattle, WA, USA., Bloom JS; Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA.; Lawrence Berkeley National Laboratory, Berkeley, CA, USA., De K; Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA., Groom SL; Infrared Processing and Analysis Center (IPAC), California Institute of Technology, Pasadena, CA, USA., Kasliwal MM; Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA., Masci FJ; Infrared Processing and Analysis Center (IPAC), California Institute of Technology, Pasadena, CA, USA., Medford MS; Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA.; Lawrence Berkeley National Laboratory, Berkeley, CA, USA., Park S; Ulsan National Institute of Science and Technology, Ulsan, South Korea., Purdum J; Caltech Optical Observatories, California Institute of Technology, Pasadena, CA, USA., Reynolds TM; The Cosmic Dawn Center (DAWN), Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Riddle R; Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA., Robert E; Univ. Lyon, Univ. Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, France., Ryder SD; School of Mathematical and Physical Sciences, Macquarie University, Sydney, New South Wales, Australia.; Astronomy, Astrophysics and Astrophotonics Research Centre, Macquarie University, Sydney, New South Wales, Australia., Sharma Y; Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA., Stern D; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
Source: Nature [Nature] 2023 May; Vol. 617 (7961), pp. 477-482. Date of Electronic Publication: 2023 May 17.
Publication Type: Journal Article; Research Support, Non-U.S. Gov't
Journal Info: Publisher: Nature Publishing Group Country of Publication: England NLM ID: 0410462 Publication Model: Print-Electronic Cited Medium: Internet ISSN: 1476-4687 (Electronic) Linking ISSN: 00280836 NLM ISO Abbreviation: Nature Subsets: MEDLINE; PubMed not MEDLINE
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  Data: A radio-detected type Ia supernova with helium-rich circumstellar material.
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