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亮暗暴的早期X射线研究
  • ISSN号：1672-7673
  • 期刊名称：《天文研究与技术》
  • 时间：0
  • 分类：P172[天文地球—天文学]
  • 作者机构：[1]厦门理工学院数理系,厦门361005南京大学天文系, [2]南京210093,南京210093
  • 相关基金：国家自然科学基金（10233010;10221001）资助. 感谢戴子高,邹远川和梁恩维的建议和修改意见：
作者： 林一清[1,2]
关键词： 亮暴, 暗暴, X射线余辉, bright GRB, sdark GRBs, X- ray afterglow
中文摘要：

研究亮暴和暗暴的X射线余辉,发现它们的X射线和γ流量的分布基本上相同。即：从统计学的角度上讲,亮暴和暗暴没有本质不同,它们的中心机制应该是相同的,暗暴的形成应该是由环境原因引起的。

英文摘要：

A systematic study on the X-ray afterglows of the optically dark and bright gamma-ray bursts is presented. Our results show that the distribution of the X-ray, the 7-ray of the dark GRBs and bright GRBs are similar, any observed differences should be caused by simply statistical fluctuation. These results indicated that the suppression of optical emission in the dark GRBs should result in the circumambiency, not in their central engine.

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期刊信息
  • 《天文研究与技术》
  • 主管单位:中国科学院
  • 主办单位:中国科学院国家天文台
  • 主编：钱声帮
  • 地址：昆明110信箱
  • 邮编：650011
  • 邮箱：ynaotk@ynao.ac.cn；
  • 电话：0871-63920157
  • 国际标准刊号：ISSN：1672-7673
  • 国内统一刊号：ISSN：53-1189/P
  • 邮发代号:
  • 获奖情况:
  • 国内外数据库收录:
  • 被引量:800