Abstract
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) 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.
| Original language | English |
|---|---|
| Article number | L16 |
| Pages (from-to) | - |
| Number of pages | 6 |
| Journal | Astrophysical Journal Letters |
| Volume | 740 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 10 Oct 2011 |
Keywords
- pulsars: individual (1E 1841-045)
- X-rays: bursts
- SOFT GAMMA-REPEATERS
- KES 73
- SUPERNOVA REMNANT
- 2002 OUTBURST
- SGR 1627-41
- 4U 0142+61
- MAGNETAR
- 1E-1841-045
- MONITOR
- DISCOVERY