Clustering of Gamma-Ray Burst Pulse Properties: A Cleaner Delineation of GRB Classes

Details Clustering of Gamma-Ray Burst Pulse Properties: A Cleaner Delineation of GRB Classes Clustering of Gamma-Ray Burst Pulse Properties: A Cleaner Delineation of GRB Classes

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21540507a&link_type=abstract

American Astronomical Society, AAS Meeting #215, #405.07; Bulletin of the American Astronomical Society, Vol. 42, p.229

Astronomy and Astrophysics

Astronomy

Scientific paper

Using a range of single- to multi-pulsed- BATSE gamma-ray bursts (GRBs),
we demonstrate that the Long GRB class can have long and short duration
pulses, whereas the Short GRB class appears to be dominated by short
duration pulses (and occasionally by unpulsed prompt emission); this
contradicts claims that Short GRBs can have long durations.

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