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作 者:YANG Yu-xuan CHE Hai-hong WU Mei CAO Sheng-lin 杨宇轩;车海红;吴枚;曹盛林(Department of Astronomy,Beijing Normal University,Beijing 100875;High Energy Astrophysics Laboratory,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100039;Shaanxi Astronomical Observatory,Chinese Academy of Sciences,Lintong 710600)
机构地区:[1]Department of Astronomy,Beijing Normal University,Beijing 100875 [2]High Energy Astrophysics Laboratory,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100039 [3]Shaanxi Astronomical Observatory,Chinese Academy of Sciences,Lintong 710600
出 处:《Chinese Physics Letters》1997年第10期797-800,共4页中国物理快报(英文版)
摘 要:Using the high time-resolution and 64ms resolution data of the burst and transient source experiment,we performed an autocorrelation analysis of the energy dependence of burst pulse width in short gamma-ray bursts.A method free from potential cosmological effects has been proposed.This allows us to use a sample with a size comparable to that used for long and bright bursts.Our result shows that the profiles of short bursts exhibit a very good power-law between profile width and photon energy,with an index~-0.3.This result is consistent with a united origin of the bimodal distribution.
关 键 词:RESOLUTION MODAL transient
分 类 号:O57[理学—粒子物理与原子核物理]
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