Fireball/Blastwave Model and Soft γ-Ray Repeaters

Fireball/Blastwave Model and Soft γ-Ray Repeaters
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火球/爆炸波模型和软 γ 射线中继器

DOI:
10.1088/0256-307x/15/10/028
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发表时间:
1998
影响因子:
3.5
通讯作者:
T. Lu
T. Lu
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
Y. F. Huang;Z. Dai;T. Lu

文献摘要

被引文献

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软γ射线中继器的距离是确定的,其位置也是准确的。如果观测到它们的软γ射线爆发的余辉,将为研究所谓的“经典γ射线爆发”提供重要线索。将经典γ射线暴的流行火球/爆炸波模型应用于软γ射线中继站,发现它们的X射线和光学余辉是可探测的。要求对三个中继器进行监测。
Soft γ-ray repeaters are at determined distances and their positions are known accurately. If observed, afterglows from their soft γ-ray bursts will provide important clues to the study of the so called "classical γ-ray bursts". On applying the popular fireball/blastwave model of classical γ-ray bursts to soft γ-ray repeaters, it is found that their x-ray and optical afterglows are detectable. Monitoring of the three repeaters is solicited.