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No supernovae associated with two long-duration γ-ray bursts

Author

Listed:
  • Johan P. U. Fynbo

    (Dark Cosmology Centre)

  • Darach Watson

    (Dark Cosmology Centre)

  • Christina C. Thöne

    (Dark Cosmology Centre)

  • Jesper Sollerman

    (Dark Cosmology Centre
    Stockholm University, AlbaNova)

  • Joshua S. Bloom

    (University of California at Berkeley)

  • Tamara M. Davis

    (Dark Cosmology Centre)

  • Jens Hjorth

    (Dark Cosmology Centre)

  • Páll Jakobsson

    (University of Hertfordshire)

  • Uffe G. Jørgensen

    (Niels Bohr Institute, University of Copenhagen)

  • John F. Graham

    (Space Telescope Science Institute)

  • Andrew S. Fruchter

    (Space Telescope Science Institute)

  • David Bersier

    (Astrophysics Research Institute, Liverpool John Moores University)

  • Lisa Kewley

    (University of Hawaii, Institute of Astronomy)

  • Arnaud Cassan

    (Astronomisches Rechen-Institut (ARI), Zentrum für Astronomie der Universität Heidelberg (ZAH))

  • José María Castro Cerón

    (Dark Cosmology Centre)

  • Suzanne Foley

    (University College Dublin)

  • Javier Gorosabel

    (Instituto de Astrofísica de Andalucía (CSIC), Apartado de Correos)

  • Tobias C. Hinse

    (Niels Bohr Institute, University of Copenhagen)

  • Keith D. Horne

    (University of St Andrews)

  • Brian L. Jensen

    (Dark Cosmology Centre)

  • Sylvio Klose

    (Thüringer Landessternwarte Tautenburg)

  • Daniel Kocevski

    (University of California at Berkeley)

  • Jean-Baptiste Marquette

    (Université Pierre et Marie Curie)

  • Daniel Perley

    (University of California at Berkeley)

  • Enrico Ramirez-Ruiz

    (Institute for Advanced Study
    University of California)

  • Maximilian D. Stritzinger

    (Dark Cosmology Centre)

  • Paul M. Vreeswijk

    (European Southern Observatory
    Universidad de Chile)

  • Ralph A. M. Wijers

    (University of Amsterdam)

  • Kristian G. Woller

    (Niels Bohr Institute, University of Copenhagen)

  • Dong Xu

    (Dark Cosmology Centre)

  • Marta Zub

    (Astronomisches Rechen-Institut (ARI), Zentrum für Astronomie der Universität Heidelberg (ZAH))

Abstract

The long and the short of it The tidy classification system that divided γ-ray bursts (GRBs) into long-duration busts (lasting more than two seconds) and short may have had its day. The final nail in its coffin may be GRB 060614. Discovered on 14 June 2006 by the Burst Alert Telescope on-board the Swift satellite, this burst was long, at 102 seconds, but as reported in a clutch of papers in this issue, it has a number of properties, including the absence of an accompanying supernova, that were previously considered diagnostic of a 'short' GRB. The hunt is now on for a classification system to take account of the diversity now apparent in GRBs. In the accompanying News & Views, Bing Zhang suggests that the answer may be to adopt a Type I/Type II classification similar to that used for supernovae.

Suggested Citation

  • Johan P. U. Fynbo & Darach Watson & Christina C. Thöne & Jesper Sollerman & Joshua S. Bloom & Tamara M. Davis & Jens Hjorth & Páll Jakobsson & Uffe G. Jørgensen & John F. Graham & Andrew S. Fruchter &, 2006. "No supernovae associated with two long-duration γ-ray bursts," Nature, Nature, vol. 444(7122), pages 1047-1049, December.
    • Handle: RePEc:nat:nature:v:444:y:2006:i:7122:d:10.1038_nature05375
    DOI: 10.1038/nature05375
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