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The prompt emission & peculiar break of GRB 060124

P. A. Curran·D. A. Kann·P. Ferrero·E. Rol·R. A. M. J. Wijers
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Abstract

Our multi-wavelength analysis of GRB 060124 shows the unusual behaviour of the decaying lightcurve as well as supporting the recently proposed phenomenon of long-lasting central engine activity. The prompt X-ray emission displays uncommonly well resolved flaring behaviour, with spectral evolution - indicative of central engine activity - which allows us to estimate the energy injection time for each flare. The otherwise smooth X-ray & optical afterglows demonstrate achromatic breaks at about 1 day which differ significantly from the usual jet break in the blastwave model of afterglows.

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P. A. Curran, D. A. Kann, P. Ferrero, E. Rol, R. A. M. J. Wijers. 2007-03-15. The prompt emission & peculiar break of GRB 060124. https://doi.org/10.1393/ncb%2Fi2007-10278-9

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