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How pulses in short gamma-ray bursts constrain HMXRB evolution

Published online by Cambridge University Press:  30 December 2019

Jon Hakkila  and
Robert D. Preece
Jon Hakkila
Affiliation:
Dept. of Physics and Astronomy, College of Charleston, 66 George St., Charleston, SC, USA email: hakkilaj@cofc.edu
Robert D. Preece
Affiliation:
Dept. of Space Science, University of Alabama in Huntsville, Huntsville, AL, USA email: rob.preece@nasa.gov
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Abstract

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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.

Keywords

X-rays: binariesgamma rays: burstsmethods: data analysismethods: statistical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S346: High-mass X-ray Binaries: Illuminating the Passage from Massive Binaries to Merging Compact Objects , August 2018 , pp. 459 - 463
Copyright
© International Astronomical Union 2019 

References

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