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- W764080355 abstract "Magnetars are slowly rotating neutron stars with extreme magnetic fields, over 10(exp 15) Gauss. Only few have been discovered in the last 30 years. These sources are dormant most of their lifetimes and become randomly active emitting multiple soft gamma-ray bursts. We present here our results on the temporal analysis of ~300 bursts from Soft Gamma Repeater SGR J1550-5418 recorded with the Gamma-ray Burst Monitor (GBM) onboard the Fermi Observatory during its activation on January 22-29, 2009. We employed an un-triggered burst search in the energy range 8-100keV to collect all events from the source, besides the ones that triggered GBM. For the entire sample of bursts we determined their durations, rise and decay times. We study here the statistical properties of these characteristics and discuss how these may help us better understand the physical characteristics of the magnetar model." @default.
- W764080355 created "2016-06-24" @default.
- W764080355 creator A5091611691 @default.
- W764080355 date "2010-01-01" @default.
- W764080355 modified "2023-09-27" @default.
- W764080355 title "Statistical Properties of SGR J1550-5418 Bursts" @default.
- W764080355 hasPublicationYear "2010" @default.
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