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Unusually rapid variability of the GRB000301C optical afterglow

  • N. Masetti
  • , C. Bartolini
  • , S. Bernabei
  • , A. Guarnieri
  • , E. Palazzi
  • , E. Pian
  • , A. Piccioni
  • , A.J. Castro-Tirado
  • , J.M.C. Ceron
  • , L. Verdes-Montenegro
  • , R. Sagar
  • , V. Mohan
  • , A.K. Pandey
  • , S.B. Pandey
  • , H. Bock
  • , J. Greiner
  • , S. Benetti
  • , R.A.M.J. Wijers
  • , G.M. Beskin
  • , J. Gorosabel

    Research output: Contribution to journalJournal articleResearchpeer-review

    Abstract

    We present BVRI light curves of the afterglow of GRB000301C, one of the brightest ever detected at a day time scale interval after GRB trigger. The monitoring started 1.5 days after the GRB and ended one month later. Inspection of the extremely well sampled R band light curve and comparison with BVI data has revealed complex behavior, with a long term flux decrease and various short time scale features superimposed. These features are uncommon among other observed afterglows. and might trace either intrinsic variability within the relativistic shock (re-acceleration and re-energization) or inhomogeneities in the medium in which the shock propagates.
    Original languageEnglish
    JournalAstronomy and Astrophysics
    Volume359
    Issue number3
    Pages (from-to)L23-L26
    ISSN0004-6361
    Publication statusPublished - 2000

    Keywords

    • gamma rays : bursts

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