Detection of a supernova signature associated with GRB 011121

  • J. S. Bloom
  • , S. R. Kulkarni
  • , P. A. Price
  • , D. Reichart
  • , T. J. Galama
  • , B. P. Schmidt
  • , D. A. Frail
  • , E. Berger
  • , P. J. McCarthy
  • , R. A. Chevalier
  • , J. C. Wheeler
  • , J. P. Halpern
  • , D. W. Fox
  • , S. G. Djorgovski
  • , F. A. Harrison
  • , R. Sari
  • , T. S. Axelrod
  • , R. A. Kimble
  • , J. Holtzman
  • , K. Hurley
  • F. Frontera, L. Piro, E. Costa

Research output: Contribution to journalArticlepeer-review

128 Scopus citations

Abstract

Using observations from an extensive monitoring campaign with the Hubble Space Telescope, we present the detection of an intermediate-time flux excess that is redder in color relative to the afterglow of GRB 011121, currently distinguished as the gamma-ray burst with the lowest known redshift. The red "bump," which exhibits a spectral rollover at ∼7200 A, is well described by a redshifted Type le supernova that occurred approximately at the same time as the gamma-ray burst event. The inferred luminosity is about half that of the bright supernova SN 1998bw. These results serve as compelling evidence for a massive star origin of long-duration gamma-ray bursts. Models that posit a supernova explosion weeks to months preceding the gamma-ray burst event are excluded by these observations. Finally, we discuss the relationship between spherical core-collapse supernovae and gamma-ray bursts.

Original languageEnglish (US)
Pages (from-to)L45-L49
JournalAstrophysical Journal
Volume572
Issue number1 II
DOIs
StatePublished - Jun 10 2002

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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