IDEAS home Printed from https://ideas.repec.org/a/nat/nature/v551y2017i7678d10.1038_nature24298.html
   My bibliography  Save this article

Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger

Author

Listed:
  • E. Pian

    (INAF, Institute of Space Astrophysics and Cosmic Physics)

  • P. D’Avanzo

    (INAF, Osservatorio Astronomico di Brera)

  • S. Benetti

    (INAF, Osservatorio Astronomico di Padova)

  • M. Branchesi

    (Gran Sasso Science Institute)

  • E. Brocato
  • S. Campana

    (INAF, Osservatorio Astronomico di Brera)

  • E. Cappellaro

    (INAF, Osservatorio Astronomico di Padova)

  • S. Covino

    (INAF, Osservatorio Astronomico di Brera)

  • V. D’Elia

    (Space Science Data Center, ASI, Via del Politecnico)

  • J. P. U. Fynbo

    (Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen)

  • F. Getman

    (INAF, Osservatorio Astronomico di Capodimonte)

  • G. Ghirlanda

    (INAF, Osservatorio Astronomico di Brera)

  • G. Ghisellini

    (INAF, Osservatorio Astronomico di Brera)

  • A. Grado

    (INAF, Osservatorio Astronomico di Capodimonte)

  • G. Greco

    (Università degli Studi di Urbino ‘Carlo Bo’
    INFN, Sezione di Firenze)

  • J. Hjorth

    (Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen)

  • C. Kouveliotou

    (Astronomy, Physics, The George Washington University, Corcoran Hall)

  • A. Levan

    (University of Warwick)

  • L. Limatola

    (INAF, Osservatorio Astronomico di Capodimonte)

  • D. Malesani

    (Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen)

  • P. A. Mazzali

    (Astrophysics Research Institute, Liverpool John Moores University, Liverpool Science Park, IC2
    Max-Planck-Institut für Astrophysik)

  • A. Melandri

    (INAF, Osservatorio Astronomico di Brera)

  • P. Møller

    (European Southern Observatory)

  • L. Nicastro

    (INAF, Institute of Space Astrophysics and Cosmic Physics)

  • E. Palazzi

    (INAF, Institute of Space Astrophysics and Cosmic Physics)

  • S. Piranomonte
  • A. Rossi

    (INAF, Institute of Space Astrophysics and Cosmic Physics)

  • O. S. Salafia

    (INAF, Osservatorio Astronomico di Brera
    Università degli Studi di Milano-Bicocca)

  • J. Selsing

    (Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen)

  • G. Stratta

    (Università degli Studi di Urbino ‘Carlo Bo’
    INFN, Sezione di Firenze)

  • M. Tanaka

    (National Astronomical Observatory of Japan)

  • N. R. Tanvir

    (University of Leicester)

  • L. Tomasella

    (INAF, Osservatorio Astronomico di Padova)

  • D. Watson

    (Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen)

  • S. Yang

    (Padova University
    University of California)

  • L. Amati

    (INAF, Institute of Space Astrophysics and Cosmic Physics)

  • L. A. Antonelli
  • S. Ascenzi

    (Università di Roma La Sapienza
    Università di Roma Tor Vergata)

  • M. G. Bernardini

    (INAF, Osservatorio Astronomico di Brera
    Laboratoire Univers et Particules de Montpellier, Université Montpellier)

  • M. Boër

    (ARTEMIS (UCA, CNRS, OCA), Boulevard de l’Observatoire, CS 34229)

  • F. Bufano

    (INAF — Osservatorio Astronomico di Catania)

  • A. Bulgarelli

    (INAF, Institute of Space Astrophysics and Cosmic Physics)

  • M. Capaccioli

    (INAF, Osservatorio Astronomico di Capodimonte
    University of Naples Federico II)

  • P. Casella
  • A. J. Castro-Tirado

    (Instituto de Astrofisica de Andalucia (CSIC), Glorieta de la Astronomia)

  • E. Chassande-Mottin

    (APC, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris)

  • R. Ciolfi

    (INAF, Osservatorio Astronomico di Padova
    INFN-TIFPA, Trento Institute for Fundamental Physics and Applications)

  • C. M. Copperwheat

    (Astrophysics Research Institute, Liverpool John Moores University, Liverpool Science Park, IC2)

  • M. Dadina

    (INAF, Institute of Space Astrophysics and Cosmic Physics)

  • G. De Cesare

    (INAF, Institute of Space Astrophysics and Cosmic Physics)

  • A. Di Paola
  • Y. Z. Fan

    (Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Science)

  • B. Gendre

    (University of Virgin Islands, 2 John Brewer’s Bay, St Thomas)

  • G. Giuffrida
  • A. Giunta
  • L. K. Hunt

    (INAF — Osservatorio Astrofisico di Arcetri)

  • G. L. Israel
  • Z.-P. Jin

    (Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Science)

  • M. M. Kasliwal

    (Mathematics and Astronomy, California Institute of Technology)

  • S. Klose

    (Thüringer Landessternwarte Tautenburg)

  • M. Lisi
  • F. Longo

    (University of Trieste and INFN Trieste)

  • E. Maiorano

    (INAF, Institute of Space Astrophysics and Cosmic Physics)

  • M. Mapelli

    (INAF, Osservatorio Astronomico di Padova
    Institute for Astrophysics and Particle Physics, University of Innsbruck)

  • N. Masetti

    (INAF, Institute of Space Astrophysics and Cosmic Physics
    Universidad Andrés Bello)

  • L. Nava

    (INAF, Osservatorio Astronomico di Brera
    INAF, Osservatorio Astronomico di Trieste, Via G.B)

  • B. Patricelli

    (Scuola Normale Superiore)

  • D. Perley

    (Astrophysics Research Institute, Liverpool John Moores University, Liverpool Science Park, IC2)

  • A. Pescalli

    (INAF, Osservatorio Astronomico di Brera
    Università degli Studi dell’Insubria)

  • T. Piran

    (Racah Institute of Physics, The Hebrew University of Jerusalem)

  • A. Possenti

    (INAF, Osservatorio Astronomico di Cagliari)

  • L. Pulone
  • M. Razzano

    (Scuola Normale Superiore)

  • R. Salvaterra

    (INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano)

  • P. Schipani

    (INAF, Osservatorio Astronomico di Capodimonte)

  • M. Spera

    (INAF, Osservatorio Astronomico di Padova)

  • A. Stamerra

    (Scuola Normale Superiore
    INAF, Osservatorio Astronomico di Torino)

  • L. Stella
  • G. Tagliaferri

    (INAF, Osservatorio Astronomico di Brera)

  • V. Testa
  • E. Troja

    (NASA, Goddard Space Flight Center)

  • M. Turatto

    (INAF, Osservatorio Astronomico di Padova)

  • S. D. Vergani

    (INAF, Osservatorio Astronomico di Brera
    GEPI, Observatoire de Paris, PSL Research University, CNRS, Place Jules Janssen)

  • D. Vergani

    (INAF, Institute of Space Astrophysics and Cosmic Physics)

Abstract

Observations of the transient associated with the gravitational-wave event GW170817 and γ-ray burst GRB 170817A reveal a bright kilonova with fast-moving ejecta, including lanthanides synthesized by rapid neutron capture.

Suggested Citation

  • E. Pian & P. D’Avanzo & S. Benetti & M. Branchesi & E. Brocato & S. Campana & E. Cappellaro & S. Covino & V. D’Elia & J. P. U. Fynbo & F. Getman & G. Ghirlanda & G. Ghisellini & A. Grado & G. Greco & , 2017. "Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger," Nature, Nature, vol. 551(7678), pages 67-70, November.
  • Handle: RePEc:nat:nature:v:551:y:2017:i:7678:d:10.1038_nature24298
    DOI: 10.1038/nature24298
    as

    Download full text from publisher

    File URL: https://www.nature.com/articles/nature24298
    File Function: Abstract
    Download Restriction: Access to the full text of the articles in this series is restricted.

    File URL: https://libkey.io/10.1038/nature24298?utm_source=ideas
    LibKey link: if access is restricted and if your library uses this service, LibKey will redirect you to where you can use your library subscription to access this item
    ---><---

    As the access to this document is restricted, you may want to search for a different version of it.

    More about this item

    Statistics

    Access and download statistics

    Corrections

    All material on this site has been provided by the respective publishers and authors. You can help correct errors and omissions. When requesting a correction, please mention this item's handle: RePEc:nat:nature:v:551:y:2017:i:7678:d:10.1038_nature24298. See general information about how to correct material in RePEc.

    If you have authored this item and are not yet registered with RePEc, we encourage you to do it here. This allows to link your profile to this item. It also allows you to accept potential citations to this item that we are uncertain about.

    We have no bibliographic references for this item. You can help adding them by using this form .

    If you know of missing items citing this one, you can help us creating those links by adding the relevant references in the same way as above, for each refering item. If you are a registered author of this item, you may also want to check the "citations" tab in your RePEc Author Service profile, as there may be some citations waiting for confirmation.

    For technical questions regarding this item, or to correct its authors, title, abstract, bibliographic or download information, contact: Sonal Shukla or Springer Nature Abstracting and Indexing (email available below). General contact details of provider: http://www.nature.com .

    Please note that corrections may take a couple of weeks to filter through the various RePEc services.

    IDEAS is a RePEc service. RePEc uses bibliographic data supplied by the respective publishers.