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Duration distributions for different softness groups of gamma-ray bursts 被引量:1

Duration distributions for different softness groups of gamma-ray bursts
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摘要 Gamma-ray bursts(GRBs) are divided into two classes according to their durations.We investigate if the softness of bursts plays a role in the conventional classification of the objects.We employ the BATSE(Burst and Transient Source Experiment) catalog and analyze the duration distributions of different groups of GRBs associated with distinct softness.Our analysis reveals that the conventional classification of GRBs with the duration of bursts is influenced by the softness of the objects.There exists a bimodality in the duration distribution of GRBs for each group of bursts and the time position of the dip in the bimodality histogram shifts with the softness parameter.Our findings suggest that the conventional classification scheme should be modified by separating the two well-known populations in different softness groups,which would be more reasonable than doing so with a single sample.According to the relation between the dip position and the softness parameter,we get an empirical function that can roughly set apart the short-hard and long-soft bursts:SP =(0.100 ± 0.028) T-(0.85 0.18) 90,± where SP is the softness parameter adopted in this paper. Gamma-ray bursts(GRBs) are divided into two classes according to their durations.We investigate if the softness of bursts plays a role in the conventional classification of the objects.We employ the BATSE(Burst and Transient Source Experiment) catalog and analyze the duration distributions of different groups of GRBs associated with distinct softness.Our analysis reveals that the conventional classification of GRBs with the duration of bursts is influenced by the softness of the objects.There exists a bimodality in the duration distribution of GRBs for each group of bursts and the time position of the dip in the bimodality histogram shifts with the softness parameter.Our findings suggest that the conventional classification scheme should be modified by separating the two well-known populations in different softness groups,which would be more reasonable than doing so with a single sample.According to the relation between the dip position and the softness parameter,we get an empirical function that can roughly set apart the short-hard and long-soft bursts:SP =(0.100 ± 0.028) T-(0.85 0.18) 90,± where SP is the softness parameter adopted in this paper.
作者 GUPTA A.C.
出处 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS 2010年第7期1375-1382,共8页 中国科学:物理学、力学、天文学(英文版)
基金 supported in part by the National Natural Science Foundation of China (Grant Nos. 10633010,10573005 and 10747001) the National Basic Research Program of China (Grant No. 2007CB815405) the financial support from the Guangzhou Education Bureau and Guangzhou Science and Technology Bureau
关键词 GAMMA-RAYS bursts:methods data analysis:methods statistical gamma-rays bursts:methods data analysis:methods statistical
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  • 1Eichler D,Livio M,Piran T,et al.Nucleosynthesis, neutrino bursts and gamma-rays from coalescing neutron stars. Nature . 1989
  • 2C. Kouveliotou,C. A. Meegan,G. J. Fishman.Identification of two classes of γ-ray bursts. The Astrophysical Journal . 1993
  • 3Fishman G J,Meegan CA.Gamma-ray bursts. Annu Rev As- tron Astrophys . 1995
  • 4Paciesas W S,Meegan C A,Pendleton G N,et al.The fourth BATSE gamma-ray burst catalog (Revised). The Astrophysical Journal Supplement Series . 1999
  • 5Qin Y P,Xie G Z,Xue S J,et al.The hardness duration correlation in the two classes of Gamma-Ray bursts. Publications Astronomical Society of Japan . 2000
  • 6Paczynski B.Gamma-ray bursters at cosmological distances. The Astrophysical Journal . 1986
  • 7Gehrels,N.,Chincarini,G.,Giommi,P.,Mason,K.O.,Nousek,J.A.The Swift gamma-ray burst mission. The Astrophysical Journal . 2004
  • 8Fruchter, A. S,Levan, A. J,Strolger, L. et al.Long gamma-ray bursts and corecollapse supernovae have different environments. Nature . 2006
  • 9Stanek,K.Z.Spectroscopic discovery of the supernova 2003dh associated with GRB 030329. The Astrophysical Journal . 2003
  • 10Hjorth J,Sollerman J,Moller P. et al.A very energetic supernova associated with the γ-ray burst of 29 March 2003. Nature . 2003

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