SHORT SOFT Г-RAY BURST SPECTRAL EVOLUTION

V. N. Kondratyev

doi:10.18524/1810-4215.2017.30.114279

Odessa Astronomical Publications (Nov 2017)

SHORT SOFT Г-RAY BURST SPECTRAL EVOLUTION

V. N. Kondratyev

Affiliations

V. N. Kondratyev: Physics Department, Taras Shevchenko National University of Kyiv, Bogolubov Laboratory of Theoretical Physics, JINR, 141980, Dubna, Russia

DOI: https://doi.org/10.18524/1810-4215.2017.30.114279
Journal volume & issue: Vol. 30, no. 0
pp. 89 – 90

Abstract

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Short Soft Gamma-Ray bursts are considered as neutron star crust magnetoemission. Statistics of temporal burst properties are shown to display univesal features.

Published in Odessa Astronomical Publications

ISSN: 1810-4215 (Print)
Publisher: Odessa I. I. Mechnykov National University
Country of publisher: Ukraine
LCC subjects: Science: Astronomy
Website: http://oap.onu.edu.ua/

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