GRB 081024B and GRB 140402A: Two Additional Short GRBs from Binary Neutron Star Mergers
Abstract
Theoretical and observational evidences for a two-fold classification of short bursts have been recently obtained: (1) short gamma-ray flashes (S-GRFs), with isotropic energy {E}{iso}< {10}52 erg and no black hole (BH) formation, and (2) authentic short gamma-ray bursts (S-GRBs), with isotropic energy {E}{iso}> {10}52 erg showing evidence of BH formation in the binary neutron star merging process. The signature for BH formation is the onset of high-energy (0.1-100 GeV) emission, coeval to the prompt emission, in all S-GRBs. No GeV emission is expected nor observed in S-GRFs. In this paper, we present two S-GRBs, GRB 081024B and GRB 140402A, in addition to the already identified S-GRBs, GRB 090227B, GRB 090510, and GRB 140619B. We also return to the absence of GeV emission in the S-GRB 090227B, at an angle of 71^\circ from the Fermi-LAT boresight. All of the correctly identified S-GRBs correlate with high-energy emission, implying no significant presence of beaming in GeV emission. The existence of a common power-law behavior in the GeV luminosities, following the BH formation, when measured in the source rest frame, points to a commonality in the mass and spin of the newly formed BHs in all S-GRBs.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- July 2017
- DOI:
- 10.3847/1538-4357/aa7a9f
- arXiv:
- arXiv:1704.08179
- Bibcode:
- 2017ApJ...844...83A
- Keywords:
-
- gamma-ray burst: general;
- gamma-ray burst: individual: GRB 081024B;
- GRB 140402A;
- stars: neutron;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 16 pages, submitted to ApJ, second version addressing the comments by the referee