articleThe Astrophysical Journal LettersOct 16, 2017BRONZE OA

The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South

RCR. ChornockEBE. BergerDKD. KasenPSP. S. CowperthwaiteMNM. Nicholl

Ohio University · Center for Astrophysics Harvard & Smithsonian · +19 more institutions

Indexed inarxivcrossrefdoaj

Abstract

Abstract We present a near-infrared spectral sequence of the electromagnetic counterpart to the binary neutron star merger GW170817 detected by Advanced Laser Interferometer Gravitational-wave Observatory (LIGO)/Virgo. Our data set comprises seven epochs of J + H spectra taken with FLAMINGOS-2 on Gemini-South between 1.5 and 10.5 days after the merger. In the initial epoch, the spectrum is dominated by a smooth blue continuum due to a high-velocity, lanthanide-poor blue kilonova component. Starting the following night, all of the subsequent spectra instead show features that are similar to those predicted in model spectra of material with a high concentration of lanthanides, including spectral peaks near 1.07…

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Authors

32
  • RC
    R. ChornockCorresponding

    Ohio University

  • EB
    E. Berger

    Center for Astrophysics Harvard & Smithsonian

  • DK
    D. Kasen

    Lawrence Berkeley National Laboratory, University of California, Berkeley

  • PS
    P. S. Cowperthwaite

    Center for Astrophysics Harvard & Smithsonian, Brandeis University

  • MN
    M. Nicholl

    Center for Astrophysics Harvard & Smithsonian

Topics & keywords

Keywords
  • Spectral line
  • Neutron star
  • Nucleosynthesis
  • Kilonova
  • Binary number
  • Observatory
  • Neutron
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