Figure 3 from NICER View of the 2020 Burst Storm and Persistent Emission of SGR 1935+2154

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

NICER View of the 2020 Burst Storm and Persistent Emission of SGR 1935+2154

Authors: George Younes, Tolga Güver, Chryssa Kouveliotou, Matthew G. Baring, Chin-Ping Hu, Zorawar Wadiasingh, Beste Begiçarslan, Teruaki Enoto, Ersin Göğüş, Lin Lin, Alice K. Harding, Alexander J. van der Horst, Walid A. Majid, Sebastien Guillot, and Christian Malacaria

2020 The Astrophysical Journal Letters 904 L21.

Provider: AAS Journals

Caption: Figure 3.

Left panel: T₉₀ distribution of the SGR 1935+2154 bursts detected during the burst storm. The black solid line is the best-fit lognormal function to the distribution with a mean of 840 ms. Middle panel: T₁₀₀ distribution along with the best-fit lognormal function (black solid line) with a mean of 1.27 s. Right panel: waiting-time distribution and the best-fit lognormal function, shown as a black solid line. The average waiting time between bursts is 2.1 s. See text for more details.

Other Images in This Article

Copyright and Terms & Conditions