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dc.contributor.authorLin, Lin
dc.contributor.authorKouveliotou, Chryssa
dc.contributor.authorGogus, Ersin
dc.contributor.authorvan der Horst, Alexander J.
dc.contributor.authorWatts, Anna L.
dc.contributor.authorBaring, Matthew G.
dc.contributor.authorKaneko, Yuki
dc.contributor.authorWijers, Ralph A. M. J.
dc.contributor.authorWoods, Peter M.
dc.contributor.authorBarthelmy, Scott
dc.contributor.authorBurgess, James Michael
dc.contributor.authorChaplin, Vandiver
dc.contributor.authorGehrels, Neil
dc.contributor.authorGoldstein, Adam
dc.contributor.authorGranot, Jonathan
dc.contributor.authorGuiriec, Sylvain
dc.contributor.authorMcenery, Julie
dc.contributor.authorPreece, Robert D.
dc.contributor.authorTierney, David
dc.contributor.authorvan der Klis, Michiel
dc.contributor.authorvon Kienlin, Andreas
dc.contributor.authorZhang, Shuang Nan
dc.date.accessioned2011-10-19T09:01:07Z
dc.date.available2011-10-19T09:01:07Z
dc.date.issued2011-10-10
dc.identifier.citationLin , L , Kouveliotou , C , Gogus , E , van der Horst , A J , Watts , A L , Baring , M G , Kaneko , Y , Wijers , R A M J , Woods , P M , Barthelmy , S , Burgess , J M , Chaplin , V , Gehrels , N , Goldstein , A , Granot , J , Guiriec , S , Mcenery , J , Preece , R D , Tierney , D , van der Klis , M , von Kienlin , A & Zhang , S N 2011 , ' Burst and persistent emission properties during the recent active episode of the anomalous x-ray pulsar 1E 1841-045 ' , Astrophysical Journal Letters , vol. 740 , no. 1 , L16 , pp. - . https://doi.org/10.1088/2041-8205/740/1/L16
dc.identifier.issn2041-8213
dc.identifier.otherPURE: 423231
dc.identifier.otherPURE UUID: b121de45-fa28-4a35-8077-ffc5ade3bbce
dc.identifier.otherWOS: 000295210900016
dc.identifier.otherScopus: 80053530534
dc.identifier.urihttp://hdl.handle.net/2299/6721
dc.descriptionCopyright American Astronomical Society
dc.description.abstractThe 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) x 10(38) 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.en
dc.format.extent6
dc.language.isoeng
dc.relation.ispartofAstrophysical Journal Letters
dc.subjectpulsars: individual (1E 1841-045)
dc.subjectX-rays: bursts
dc.subjectSOFT GAMMA-REPEATERS
dc.subjectKES 73
dc.subjectSUPERNOVA REMNANT
dc.subject2002 OUTBURST
dc.subjectSGR 1627-41
dc.subject4U 0142+61
dc.subjectMAGNETAR
dc.subject1E-1841-045
dc.subjectMONITOR
dc.subjectDISCOVERY
dc.titleBurst and persistent emission properties during the recent active episode of the anomalous x-ray pulsar 1E 1841-045en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1088/2041-8205/740/1/L16
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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