Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-06-25
Chin.Phys.Lett. 16 (1999) 775
Astronomy and Astrophysics
Astrophysics
9 pages, aasms4 style, 3 ps figures, minor changes, will be published in Chin. Phys. Lett
Scientific paper
Conventional dynamic model of gamma-ray burst remnants is found to be incorrect for adiabatic blastwaves during the non-relativistic phase. A new model is derived, which is shown to be correct for both radiative and adiabatic blastwaves during both ultra-relativistic and non-relativistic phase. Our model also takes the evolution of the radiative efficiency into account. The importance of the transition from the ultra-relativistic phase to the non-relativistic phase is stressed.
Dai Gao Z.
Huang Yun-Feng
Lu Tan
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