Variability of the giant X-ray bump in GRB 121027A and its possible origin

The giant X-ray bump of GRB 121027A observed by Swift is different from the typical X-ray flares in gamma-ray bursts. The observed structural variability in the rise and decay phases of the bump has four components. Of these four components, only the data in the bump from about 5300 to about 6100 s...

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Published inMonthly notices of the Royal Astronomical Society Vol. 441; no. 3; pp. 2375 - 2379
Main Authors Hou, Shu-Jin, Gao, He, Liu, Tong, Gu, Wei-Min, Lin, Da-Bin, Li, Ya-Ping, Men, Yun-Peng, Wu, Xue-Feng, Lei, Wei-Hua, Lu, Ju-Fu
Format Journal Article
LanguageEnglish
Published London Oxford University Press 01.07.2014
Subjects
Correlation analysis
Gamma ray astronomy
Star & galaxy formation
X-ray astronomy
black hole physics
accretion, accretion discs
gamma-ray burst: individual: GRB 121027A
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Summary:The giant X-ray bump of GRB 121027A observed by Swift is different from the typical X-ray flares in gamma-ray bursts. The observed structural variability in the rise and decay phases of the bump has four components. Of these four components, only the data in the bump from about 5300 to about 6100 s is of good enough quality to be analysed using the stepwise filter correlation method. A $86^{+5.9}_{-9.4} \rm s$ periodic oscillation is postulated, which is confirmed by the Lomb–Scargle method. A jet precession model is proposed to account for this variability.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stu682