A new definition of the intermediate group of gamma-ray bursts

Authors: I. Horvath, L.G. Balazs, Z. Bagoly, F. Ryde, A. Meszaros
(Submitted on 30 Sep 2005 (v1), last revised 24 Oct 2005 (this version, v2))
Abstract: Gamma-ray bursts can be divided into three groups ("short", "intermediate", "long") with respect to their durations. This classification is somewhat imprecise, since the subgroup of intermediate duration has an admixture of both short and long bursts. In this paper a physically more reasonable definition of the intermediate group is presented, using also the hardnesses of the bursts. It is shown again that the existence of the three groups is real, no further groups are needed. The intermediate group is the softest one. From this new definition it follows that 11% of all bursts belong to this group. An anticorrelation between the hardness and the duration is found for this subclass in contrast to the short and long groups. Despite this difference it is not clear yet whether this group represents a physically different phenomenon.

Class membership of the bursts:

file t90h32.3

Comments: accepted for publication in Astronomy and Astrophysics
Subjects: Astrophysics (astro-ph)
Journal reference: Astron.Astrophys. 447 (2006) 23-30
DOI: 10.1051/0004-6361:20041129
Cite as: arXiv:astro-ph/0509909
  (or arXiv:astro-ph/0509909v2 for this version)