Fermi-GBM Observations of the SGR J1935+2154 Burst Forest
arXiv:2106.14172 · doi:10.3847/2041-8213/ac0fe7
Abstract
During 2020 April and May, SGR J1935+2154 emitted hundreds of short bursts and became one of the most prolific transient magnetars. At the onset of the active bursting period, a 130 s burst "forest," which included some bursts with peculiar time profiles, were observed with the Fermi/Gamma-ray Burst Monitor (GBM). In this Letter, we present the results of time-resolved spectral analysis of this burst "forest" episode, which occurred on 2020 April 27. We identify thermal spectral components prevalent during the entire 130 s episode; high-energy maxima appear during the photon flux peaks, which are modulated by the spin period of the source. Moreover, the evolution of the spectral hardness (represented by or blackbody temperature) within the lightcurve peaks is anti-correlated with the pulse phases extrapolated from the pulsation observed within the persistent soft X-ray emission of the source six hours later. Throughout the episode, the emitting area of the high-energy (hotter) component is 1-2 orders of magnitude smaller than that for the low-energy component. We interpret this with a geometrical viewing angle scenario, inferring that the high-energy component likely originates from a low-altitude hotspot located within closed toroidal magnetic field lines.
arXiv comment23 pages, 8 figures, 1 table (machine-readable table provided separately), Matches the published version
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- Insight-HXMT dedicated 33-day observation of SGR J1935+2154 II. Burst Spectral Catalog
- Direct Emission of Strong Radio Pulses During Magnetar Flares
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