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27 April 2024 |
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Evolution of the Low-Energy Photon Spectra in Gamma-Ray Bursts | A. Crider
; E. P. Liang
; I. A. Smith
; R. D. Preece
; M. S. Briggs
; G. N. Pendleton
; W. S. Paciesas
; D. L. Band
; J. L. Matteson
; | Date: |
11 Dec 1996 | Journal: | Astrophys.J. 479 (1997) 39 DOI: 10.1086/310574 | Subject: | astro-ph | Abstract: | We report evidence that the asymptotic low-energy power law slope alpha (below the spectral break) of BATSE gamma-ray burst photon spectra evolves with time rather than remaining constant. We find a high degree of positive correlation exists between the time-resolved spectral break energy E_pk and alpha. In samples of 18 "hard-to-soft" and 12 "tracking" pulses, evolution of alpha was found to correlate with that of the spectral break energy E_pk at the 99.7% and 98% confidence levels respectively. We also find that in the flux rise phase of "hard-to-soft" pulses, the mean value of alpha is often positive and in some bursts the maximum value of alpha is consistent with a value > +1. BATSE burst 3B 910927, for example, has a alpha_max equal to 1.6 +/- 0.3. These findings challenge GRB spectral models in which alpha must be negative of remain constant. | Source: | arXiv, astro-ph/9612118 | Services: | Forum | Review | PDF | Favorites |
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