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astro-ph.HEMay 31, 2019
authors
  • Jon Hakkila
  • Robert D. Preece
institutions
  • College of Charleston
  • University of Alabama in Huntsville
arXiv abstractPDF
paper

How Pulses in Short Gamma-Ray Bursts Constrain HMXRB Evolution

arXiv:1906.00015 · doi:10.1017/S1743921318007603

Abstract

We demonstrate how pulse structures in Short gamma-ray bursts (SGRBs), coupled with observations of GRB/GW 170817A, constrain the geometries of dying HMXRB systems composed of merging neutron stars.

arXiv comment5 pages, 8 figures

References in corpus (8)

  • Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
  • An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
  • Long-lag, Wide-Pulse Gamma-Ray Bursts
  • The multi-messenger picture of compact object encounters: binary mergers versus dynamical collisions
  • Gamma-Ray Burst Pulse Shapes: Evidence for Embedded Shock Signatures?
  • Properties of Short Gamma-Ray Burst Pulses from A BATSE TTE GRB Pulse Catalog
  • Determine the Lorentz factor and the viewing angle of GRB 170817A
  • Smoke and Mirrors: Signal-to-Noise and Time-Reversed Structures in Gamma-Ray Burst Pulse Light Curves
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