Reclassification of gamma-ray bursts

被引:62
作者
Balastegui, A
Ruiz-Lapuente, P
Canal, R
机构
[1] Univ Barcelona, Dept Astron & Meteomol, E-08028 Barcelona, Spain
[2] Max Planck Inst Astrophys, D-85740 Munich, Germany
[3] Inst Estudis Espacials Catalunya, Barcelona 08034, Spain
关键词
methods : data analysis; methods : statistical; gamma-rays : bursts;
D O I
10.1046/j.1365-8711.2001.04888.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have applied two different automatic classifier algorithms to the BATSE Current GRB Catalog data and we obtain three different classes of gamma-ray bursts (GRBs). Our results confirm the existence of a third, intermediate class of GRBs, with mean duration similar to 25-50 s, as deduced from a cluster analysis and from a neural network algorithm. Our analyses imply longer durations than those found by Mukherjee et al. and Horvath, whose intermediate class had durations similar to2-10 s. From the neural network analysis no difference in hardness between the two longest classes is found, and from both methods we find that the intermediate-duration class constitutes the most homogeneous sample of GRBs in its space distribution, while the longest-duration class constitutes the most inhomogeneous one with [V/V-max] similar to 0.1, being thus the deepest population of GRBs with z(max) similar to 10. The trend previously found in long bursts, of spatial inhomogeneity increasing with hardness, only holds for this new longest-duration class.
引用
收藏
页码:283 / 290
页数:8
相关论文
共 43 条
[1]  
[Anonymous], APJ
[2]  
[Anonymous], 1973, Astrophysical Journal Letters
[3]   A principal component analysis of the 3B gamma-ray burst data [J].
Bagoly, Z ;
Meszaros, A ;
Horvath, I ;
Balazs, LG ;
Meszaros, P .
ASTROPHYSICAL JOURNAL, 1998, 498 (01) :342-348
[4]   Gamma ray bursts from superconducting cosmic strings [J].
Berezinsky, V ;
Hnatyk, B ;
Vilenkin, A .
PHYSICAL REVIEW D, 2001, 64 (04)
[5]  
BLINNIKOV SI, 1999, ASTROPH9902305
[6]  
BLOOM J, 2000, ASTROPH0010176
[7]  
CASTROTIRADO AJ, 2001, ASTROPH0102122
[8]   Gamma-ray bursts from internal shocks in a relativistic wind: temporal and spectral properties [J].
Daigne, F ;
Mochkovitch, R .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1998, 296 (02) :275-286
[9]   The hardness-intensity correlation in bright gamma-ray bursts [J].
Dezalay, JP ;
Atteia, JL ;
Barat, C ;
Boer, M ;
Darracq, F ;
Goupil, P ;
Niel, M ;
Talon, R ;
Vedrenne, G ;
Hurley, K ;
Terekhov, O ;
Sunyaev, R ;
Kuznetsov, A .
ASTROPHYSICAL JOURNAL, 1997, 490 (01) :L17-L20
[10]  
FISHMAN GJ, 1999, APJS, V122, P465