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Burst and Persistent Emission Properties during the Recent Active Episode of the Anomalous X-Ray Pulsar 1E 1841-045

Lin, Lin (author)
Kouveliotou, Chryssa (author)
Göğüş, Ersin (author)
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van der Horst, Alexander J (author)
Watts, Anna L (author)
Baring, Matthew G (author)
Kaneko, Yuki (author)
Wijers, Ralph A M J (author)
Woods, Peter M (author)
Barthelmy, Scott (author)
Burgess, James Michael (author)
University of Alabama in Huntsville, United States
Chaplin, Vandiver (author)
Gehrels, Neil (author)
Goldstein, Adam (author)
Granot, Jonathan (author)
Guiriec, Sylvain (author)
McEnery, Julie (author)
Preece, Robert D (author)
Tierney, David (author)
van der Klis, Michiel (author)
von Kienlin, Andreas (author)
Zhang, Shuang Nan (author)
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 (creator_code:org_t)
Institute of Physics (IOP), 2011
2011
English.
In: Astrophysical Journal Letters. - : Institute of Physics (IOP). - 2041-8205 .- 2041-8213. ; 740:1
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The Swift/Burst Alert Telescope detected the first burst from 1E 1841-045 in 2010 May with intermittent burst activity recorded through at least 2011 July. Here we present Swift and Fermi/Gamma-ray Burst Monitor observations of this burst activity and search for correlated changes to the persistent X-ray emission of the source. The T 90 durations of the bursts range between 18 and 140 ms, comparable to other magnetar burst durations, while the energy released in each burst ranges between (0.8-25) × 1038 erg, which is on the low side of soft gamma repeater bursts. We find that the bursting activity did not have a significant effect on the persistent flux level of the source. We argue that the mechanism leading to this sporadic burst activity in 1E 1841-045 might not involve large-scale restructuring (either crustal or magnetospheric) as seen in other magnetar sources.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

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