Properties of Swift`s intermediate bursts

Details Properties of Swift`s intermediate bursts Properties of Swift`s intermediate bursts

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1358..251v&link_type=abstract

GAMMA RAY BURSTS 2010. AIP Conference Proceedings, Volume 1358, pp. 251-254 (2011).

Physics

1

Redshift, Gamma-Rays, Brightness, Spectral Analysis, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Gamma-Ray, Magnitudes And Colors, Luminosities, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification

Scientific paper

Based on their prompt, high-energy emission, gamma-ray bursts are usually classified into short-duration and long-duration classes. A third intermediate group has been identified on statistical grounds but its individual properties have not yet been studied in detail. Using the large sample of follow-up observations of GRBs produced during the Swift era we analyze the individual characteristics of this group. We find that intermediate bursts are significantly different from short GRBs but share many properties with long bursts, probably pointing to a common progenitor type. However, we find that intermediate bursts are significantly dimmer and have on average lower redshifts.

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