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首页> 外文期刊>The Astrophysical journal >A GAMMA-RAY BURST WITH A 220 MICROSECOND RISE TIME AND A SHARP SPECTRAL CUTOFF
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A GAMMA-RAY BURST WITH A 220 MICROSECOND RISE TIME AND A SHARP SPECTRAL CUTOFF

机译:伽马射线爆发,上升时间为220微秒,锐利的光谱截止

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摘要

The gamma-ray burst GRB 920229 has four extreme and unprecedented properties: a spike near the end of the burst has a rise in brightness with an e-folding timescale of 220 ±30 μs, a fall in brightness with an e- folding timescale of 400 ±100 μs, and a large change in spectral shape over a time of 768 μs, while the spectrum of the entire burst has a sharp spectral cutoff to high energies with ΔE/E = 18 . The rapid changes occur during a spike in the light curve that was seen 0.164 s after the start of the burst. The spectrum has a peak νF_v at 200 keV with no significant flux above 239 keV, although the cutoff energy shifts to less than 100 keV during the decay of the spike. These numbers can be used to place severe limits on fireball models of bursts. The thickness of the energy production region must be smaller than ~66 km, ejected shells inust have a dispersion of the Lorentz factor of less than roughly 1 along a particular radius, and the angular size of the radiation emission region is on the order of 1′as viewed from the burst center The physical mechanism that caused the sharp spectral cutoff has not been determined.
机译:伽玛射线暴GRB 920229具有四个极端和空前的特性:猝发末尾的尖峰的电子折叠时间标度为220±30μs,亮度增加;电子折叠时间标度为220±30μs,亮度下降。 400±100μs,并且在768μs的时间内光谱形状发生较大变化,而整个猝发的光谱对ΔE/ E = 18的高能量具有急剧的光谱截止。快速变化发生在爆发开始后0.164 s的光曲线尖峰期间。该频谱在200 keV处有一个峰νF_v,在239 keV以上没有明显的通量,尽管在尖峰衰减期间截止能量转移到小于100 keV。这些数字可用于对火球爆发模型进行严格限制。能量产生区域的厚度必须小于〜66 km,射出的壳沿特定半径的洛伦兹因子的色散大约小于1,并且辐射发射区域的角大小约为1从爆发中心看尚未确定引起光谱急剧截止的物理机制。

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