On the nature of the short-duration GRB 050906
Levan, A. J., Tanvir, N. R., Jakobsson, P., Chapman, R., Hjorth, J., Priddey, R. S., Fynbo, J. P. U., Hurley, K., Jensen, B. L., Johnson, R., Gorosabel, J., Castro-Tirado, A. J., Jarvis, M., Watson, D. and Wiersema, K.. (2008) On the nature of the short-duration GRB 050906. Monthly Notices of the Royal Astronomical Society, Vol.384 (No.2). pp. 541-547. ISSN 0035-8711Full text not available from this repository.
Official URL: http://dx.doi.org/10.1111/j.1365-2966.2007.11953.x
We present deep optical and infrared (IR) observations of the short-duration GRB 050906. Although no X-ray or optical/IR afterglow was discovered to deep limits, the error circle of the gamma-ray burst (GRB) (as derived from the Swift Burst Alert Telescope, or BAT) is unusual in containing the relatively local starburst galaxy IC328. This makes GRB 050906 a candidate burst from a soft gamma-ray repeater (SGR), similar to the giant flare from SGR 1806-20. The probability of chance alignment of a given BAT position with such a galaxy is small (less than or similar to 1 per cent), although the size of the error circle (2.6 arcmin radius) is such that a higher z origin cannot be ruled out. Indeed, the error circle also includes a moderately rich galaxy cluster at z = 0.43, which is a plausible location for the burst given the apparent preference that short-duration GRBs have for regions of high mass density. No residual optical or IR emission has been observed, in the form of either an afterglow or a later time emission from any associated supernova-like event. We discuss the constraints these limits place on the progenitor of GRB 050906 based on the expected optical signatures from both SGRs and merging compact object systems.
|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|
|Date:||21 February 2008|
|Number of Pages:||7|
|Page Range:||pp. 541-547|
|Access rights to Published version:||Restricted or Subscription Access|
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