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The unusual X-ray light curve of GRB 080307: the onset of the afterglow?

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Page, K. L., Willingale, R, O'Brien, P. T., Tanvir, N. R., Osborne, J. P., Zhang, B., Holland, S. T., Levan, A. J., Melandri, A., Starling, R. L. C., Bersier, D., Burrows, D. N., Geach, J. E. and Maxted, P. F. L.. (2009) The unusual X-ray light curve of GRB 080307: the onset of the afterglow? Monthly Notices of the Royal Astronomical Society, Vol.395 (No.1). pp. 328-334. ISSN 0035-8711

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Official URL: http://dx.doi.org/10.1111/j.1365-2966.2009.14509.x

Abstract

Swift-detected GRB080307 showed an unusual smooth rise in its X-ray light curve around 100 s after the burst, at the start of which the emission briefly softened. This 'hump' has a longer duration than is normal for a flare at early times and does not demonstrate a typical flare profile. Using a two-component power-law-to-exponential model, the rising emission can be modelled as the onset of the afterglow, something which is very rarely seen in Swift-X-ray light curves. We cannot, however, rule out that the hump is a particularly slow early-time flare, or that it is caused by upscattered reverse shock electrons.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science > Physics
Journal or Publication Title: Monthly Notices of the Royal Astronomical Society
Publisher: Wiley-Blackwell Publishing, Inc
ISSN: 0035-8711
Date: 1 May 2009
Volume: Vol.395
Number: No.1
Number of Pages: 7
Page Range: pp. 328-334
Identification Number: 10.1111/j.1365-2966.2009.14509.x
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
URI: http://wrap.warwick.ac.uk/id/eprint/28121

Data sourced from Thomson Reuters' Web of Knowledge

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