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A luminous blue kilonova and an off-axis jet from a compact binary merger at z = 0.1341

Author

Listed:
  • E. Troja

    (University of Maryland
    NASA Goddard Space Flight Center)

  • G. Ryan

    (University of Maryland)

  • L. Piro

    (INAF, Istituto di Astrofisica e Planetologia Spaziali)

  • H. Eerten

    (University of Bath, Claverton Down)

  • S. B. Cenko

    (NASA Goddard Space Flight Center
    University of Maryland)

  • Y. Yoon

    (Seoul National University)

  • S.-K. Lee

    (Seoul National University)

  • M. Im

    (Seoul National University)

  • T. Sakamoto

    (Aoyama Gakuin University)

  • P. Gatkine

    (University of Maryland)

  • A. Kutyrev

    (University of Maryland
    NASA Goddard Space Flight Center)

  • S. Veilleux

    (University of Maryland
    University of Maryland)

Abstract

The recent discovery of a gamma-ray burst (GRB) coincident with the gravitational-wave (GW) event GW170817 revealed the existence of a population of low-luminosity short duration gamma-ray transients produced by neutron star mergers in the nearby Universe. These events could be routinely detected by existing gamma-ray monitors, yet previous observations failed to identify them without the aid of GW triggers. Here we show that GRB150101B is an analogue of GRB170817A located at a cosmological distance. GRB150101B is a faint short burst characterized by a bright optical counterpart and a long-lived X-ray afterglow. These properties are unusual for standard short GRBs and are instead consistent with an explosion viewed off-axis: the optical light is produced by a luminous kilonova, while the observed X-rays trace the GRB afterglow viewed at an angle of ~13°. Our findings suggest that these properties could be common among future electromagnetic counterparts of GW sources.

Suggested Citation

  • E. Troja & G. Ryan & L. Piro & H. Eerten & S. B. Cenko & Y. Yoon & S.-K. Lee & M. Im & T. Sakamoto & P. Gatkine & A. Kutyrev & S. Veilleux, 2018. "A luminous blue kilonova and an off-axis jet from a compact binary merger at z = 0.1341," Nature Communications, Nature, vol. 9(1), pages 1-10, December.
  • Handle: RePEc:nat:natcom:v:9:y:2018:i:1:d:10.1038_s41467-018-06558-7
    DOI: 10.1038/s41467-018-06558-7
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