scholarly journals BATSE observations of gamma-ray burst spectra. 2: Peak energy evolution in bright, long bursts

1995 ◽  
Vol 439 ◽  
pp. 307 ◽  
Author(s):  
L. A. Ford ◽  
D. L. Band ◽  
J. L. Matteson ◽  
M. S. Briggs ◽  
G. N. Pendleton ◽  
...  
1995 ◽  
Vol 7 (3) ◽  
pp. 697-704 ◽  
Author(s):  
L Z Zhang ◽  
B Q Zong ◽  
B R Zhang ◽  
Z H Xu ◽  
J Q Li ◽  
...  

2004 ◽  
Vol 609 (2) ◽  
pp. 935-951 ◽  
Author(s):  
D. Yonetoku ◽  
T. Murakami ◽  
T. Nakamura ◽  
R. Yamazaki ◽  
A. K. Inoue ◽  
...  

2004 ◽  
Vol 616 (1) ◽  
pp. 331-338 ◽  
Author(s):  
Giancarlo Ghirlanda ◽  
Gabriele Ghisellini ◽  
Davide Lazzati

Science ◽  
2013 ◽  
Vol 343 (6166) ◽  
pp. 51-54 ◽  
Author(s):  
R. Preece ◽  
J. Michael Burgess ◽  
A. von Kienlin ◽  
P. N. Bhat ◽  
M. S. Briggs ◽  
...  

Gamma-ray burst (GRB) 130427A is one of the most energetic GRBs ever observed. The initial pulse up to 2.5 seconds is possibly the brightest well-isolated pulse observed to date. A fine time resolution spectral analysis shows power-law decays of the peak energy from the onset of the pulse, consistent with models of internal synchrotron shock pulses. However, a strongly correlated power-law behavior is observed between the luminosity and the spectral peak energy that is inconsistent with curvature effects arising in the relativistic outflow. It is difficult for any of the existing models to account for all of the observed spectral and temporal behaviors simultaneously.


2004 ◽  
Vol 606 (1) ◽  
pp. L33-L36 ◽  
Author(s):  
Ryo Yamazaki ◽  
Kunihito Ioka ◽  
Takashi Nakamura

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