Fireball/Blastwave Model and Soft γ-Ray Repeaters  

作　　者：HUANG Yong-feng DAI Zi-gao LU Tan 黄永锋;戴子高;陆琰(Department of Astronomy,Nanjing University,Nanjing 210093)

机构地区：[1]Department of Astronomy,Nanjing University,Nanjing 210093

出　　处：《Chinese Physics Letters》1998年第10期775-777,共3页中国物理快报（英文版）

基　　金：Supported by the National Natural Science Foundation of China under Grant Nos.19573006 and 19773007;the Foundation of the National Education Commit tee of China.

摘　　要：Softγ-ray repeaters are at determined distances and their positions are known accurately.If observed,afterglows from their softγ-ray bursts will provide important clues to the study of the so called“classicalγ-ray bursts”.On applying the popular fireball/blastwave model of classicalγ-ray bursts to softγ-ray repeaters,it is found that their x-ray and optical afterglows are detectable.Monitoring of the three repeaters is solicited.

关 键 词：BURSTS wave OBSERVED 

分 类 号：P14[天文地球—天体物理]