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Asymmetric mass ratios for bright double neutron-star mergers.
Ferdman, R D; Freire, P C C; Perera, B B P; Pol, N; Camilo, F; Chatterjee, S; Cordes, J M; Crawford, F; Hessels, J W T; Kaspi, V M; McLaughlin, M A; Parent, E; Stairs, I H; van Leeuwen, J.
Afiliação
  • Ferdman RD; Faculty of Science, University of East Anglia, Norwich, UK. r.ferdman@uea.ac.uk.
  • Freire PCC; Max-Planck-Institut für Radioastronomie, Bonn, Germany.
  • Perera BBP; Arecibo Observatory, Arecibo, Puerto Rico.
  • Pol N; Department of Physics and Astronomy, West Virginia University, Morgantown, WV, USA.
  • Camilo F; Center for Gravitational Waves and Cosmology, West Virginia University, Morgantown, WV, USA.
  • Chatterjee S; South African Radio Astronomy Observatory, Cape Town, South Africa.
  • Cordes JM; Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY, USA.
  • Crawford F; Department of Astronomy, Cornell University, Ithaca, NY, USA.
  • Hessels JWT; Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY, USA.
  • Kaspi VM; Department of Astronomy, Cornell University, Ithaca, NY, USA.
  • McLaughlin MA; Department of Physics and Astronomy, Franklin and Marshall College, Lancaster, PA, USA.
  • Parent E; Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, The Netherlands.
  • Stairs IH; ASTRON, Netherlands Institute for Radio Astronomy, Dwingeloo, The Netherlands.
  • van Leeuwen J; Department of Physics, McGill University, Montreal, Quebec, Canada.
Nature ; 583(7815): 211-214, 2020 07.
Article em En | MEDLINE | ID: mdl-32641814
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Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article
Texto completo
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Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article