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arxiv: 1309.0454 · v1 · pith:FZNTYVJ5new · submitted 2013-09-02 · 🌌 astro-ph.HE

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

classification 🌌 astro-ph.HE
keywords emissiongamma-raygrbsinducedsubclassx-rayaccretingassociated
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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.

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