Low Redshift GRBS and Their Host Galaxies

Details Low Redshift GRBS and Their Host Galaxies Low Redshift GRBS and Their Host Galaxies

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.2012t&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

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There is growing evidence that a proportion of GRB-like events occur at relatively low redshifts and have lower luminosities than the cosmological GRBs. Some of these are long-duration bursts which are associated with type-Ibc supernovae, and presumably produced by a similar mechanism to their higher redshift counterparts. Others are short-duration bursts which may well be produced by flares from soft gamma-ray repeaters (SGRs). I review the evidence for the existence of these various populations, and discuss the implications for progenitor models and their relative number densities.

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