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|Title:||The unusual X-ray emission of the short Swift GRB 090515: Evidence for the formation of a magnetar?|
O'Brien, P. T.
Tanvir, N. R.
Evans, P. A.
Page, K. L.
Beardmore, A. P.
Levan, A. J.
Tunnicliffe, R. L.
Burrows, D. N.
Fox, D. B.
Ukwatta, T. N.
Ukwatta, T. N.
Fruchter, A. S.
|Publisher:||Oxford University Press|
|Citation:||Monthly Notices of the Royal Astronomical Society, 2010, 409 (2), pp. 531-540|
|Abstract:||The majority of short gamma-ray bursts (SGRBs) are thought to originate from the merger of compact binary systems collapsing directly to form a black hole. However, it has been proposed that both SGRBs and long gamma-ray bursts (LGRBs) may, on rare occasions, form an unstable millisecond pulsar (magnetar) prior to final collapse. GRB 090515, detected by the Swift satellite was extremely short, with a T[subscript: 90] of 0.036 ± 0.016 s, and had a very low fluence of 2 × 10 [superscript: −8] erg cm [superscript: −2] and faint optical afterglow. Despite this, the 0.3–10 keV flux in the first 200 s was the highest observed for an SGRB by the Swift X-ray Telescope (XRT). The X-ray light curve showed an unusual plateau and steep decay, becoming undetectable after ∼500 s. This behaviour is similar to that observed in some long bursts proposed to have magnetars contributing to their emission. In this paper, we present the Swift observations of GRB 090515 and compare it to other gamma-ray bursts (GRBs) in the Swift sample. Additionally, we present optical observations from Gemini, which detected an afterglow of magnitude 26.4 ± 0.1 at T+ 1.7 h after the burst. We discuss potential causes of the unusual 0.3–10 keV emission and suggest it might be energy injection from an unstable millisecond pulsar. Using the duration and flux of the plateau of GRB 090515, we place constraints on the millisecond pulsar spin period and magnetic field.|
|Rights:||This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2010 The Authors. Journal compilation © 2010 RAS. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Deposited with reference to the publisher’s open access archiving policy.|
|Appears in Collections:||Published Articles, Dept. of Physics and Astronomy|
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