Published in
Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 2(402), p. 705-712, 2010
DOI: 10.1111/j.1365-2966.2009.15538.x
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Can X-ray emission powered by a spinning-down magnetar explain some gamma-ray burst light-curve features?
Journal article published in 2010 by
N. Lyons,
P. T. O'Brien,
B. Zhang 
,
R. Willingale,
E. Troja ,
R. L. C. Starling
,
R. Willingale,
E. Troja ,
R. L. C. Starling
This paper was not found in any repository, but could be made available legally by the author.
Full text: Unavailable
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