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Evidence for two distinct morphological classes of gamma-ray bursts from their short time scale variabilityWe have analyzed the 241 bursts for which peak counts (C)max exist in the publicly available Burst and Transient Source Experiment (BATSE) catalog. Introducing peak counts in 1024 ms as a measure of burst brightness B and the ratio of peak counts in 64 and 1024 ms as a measure of short timescale variability V, we find a statistically significant correlation between the brightness and the short time scale variability of gamma-ray bursts. The bursts which are smoother on short time scales are both faint and bright, while the bursts which are variable on short time scales are faint only, suggesting the existence of two distinct morphological classes of bursts.
Document ID
19930068018
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lamb, D. Q.
(NASA Headquarters Washington, DC United States)
Graziani, C.
(NASA Headquarters Washington, DC United States)
Smith, I. A.
(Chicago Univ. IL, United States)
Date Acquired
August 16, 2013
Publication Date
August 10, 1993
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters
Volume: 413
Issue: 1
ISSN: 0004-637X
Subject Category
Space Radiation
Accession Number
93A52015
Funding Number(s)
CONTRACT_GRANT: NAGW-1284
CONTRACT_GRANT: NAGW-830
CONTRACT_GRANT: NAG5-1454
CONTRACT_GRANT: NASW-4690
Distribution Limits
Public
Copyright
Other

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