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On a novel distance indicator for Gamma-Ray Bursts associated with Supernovae

It has been proposed that the temporal coincidence of a gamma-ray burst (GRB) and a type Ib/c supernova (SN) can be explained with the concept of induced gravitational collapse (IGC), induced by the matter ejected from an SN Ib/c accreting onto a neutron star (NS). We found a standard luminosity light curve behavior in the late-time X-ray emission of this subclass of GRBs. We interpret this as the result of a common physical mechanism in this particular phase of the X-ray emission, possibly related to the creation of the NS from the SN process. Moreover, this scaling law could be a fundamental tool for estimating the redshift of GRBs that belong to this subclass of events.

preprint2013arXivOpen access
Giovanni Battista PisaniLuca IzzoRemo RuffiniCarlo Luciano BiancoMarco MuccinoAna Virginia PenacchioniJorge Armando RuedaYu Wang
astro-ph.HE
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Giovanni Battista PisaniLuca IzzoRemo RuffiniCarlo Luciano BiancoMarco MuccinoAna Virginia PenacchioniJorge Armando RuedaYu Wang

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