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Gamma-ray Burst Spectrum Influenced by the Doppler Effect of Fireballs

Published online by Cambridge University Press:  26 May 2016

Yi-Ping Qin
Yi-Ping Qin*
Affiliation:
Yunnan Observatory, National Astronomical Observatories, CAS, Kunming, Yunnan 650011, P. R. China

Abstract

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The formula of the Doppler effect of fireballs, which shows how the observational flux from fireballs would be expected, is presented. It shows, when the expansion speed is very large, a weak radiation at X-ray bands would be significantly enhanced to detectable levels and shifted to much higher bands to become a gamma-ray source; at the same time, the peak of the spectrum would shift to a much higher energy band as well.

Type
Part 9 Gamma Ray Bursters
Information
Symposium - International Astronomical Union , Volume 214: High Energy Processes and Phenomena in Astrophysics , 2003 , pp. 335 - 338
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Band, D. et al. 1993, ApJ, 413, 281 Google Scholar
Brainerd, J. J. et al. 1998, ApJ, 501, 325 Google Scholar
Ford, L. A. et al. 1995, ApJ, 439, 307 Google Scholar
Goodman, J. 1986, ApJ, 308, L47 Google Scholar
Klebesadel, R., Strong, I., & Olson, R. 1973, ApJ, 182, L85 CrossRefGoogle Scholar
Mallozzi, R. S. et al. 1995, ApJ, 454, 597 Google Scholar
Meszaros, P. & Rees, M. J. 1998, ApJ, 502, L105 Google Scholar
Paczynski, B. 1986, ApJ, 308, L43 CrossRefGoogle Scholar
Piran, T. et al. 1993, MNRAS, 263, 861 Google Scholar
Preece, R. D. et al. 1998, ApJ, 496, 849 Google Scholar
Preece, R. D. et al. 2000, ApJS, 126, 19 Google Scholar