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HYDRODYNAMIC PROPERTIES OF GAMMA-RAY BURSTS OUTFLOWS DEDUCED FROM THE THERMAL COMPONENT
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Number of Authors: 8
2015 (English)In: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 813, no 2, 127Article in journal (Refereed) Published
Abstract [en]

We study the properties of a significant thermal emission component that was identified in 47 gamma-ray bursts observed by different instruments. Within the framework of the fireball model, we deduce the values of the Lorentz factor Gamma, and the acceleration radius, r(0), for these bursts. We find that all the values of Gamma in our sample are in the range 10(2) <= Gamma <= 10(3), with <Gamma > = 370. We find a very weak dependence of Gamma on the acceleration radius r0, Gamma proportional to r(0)(alpha) with alpha - -0.10 +/- 0.09 at the sigma - 2.1 confidence level. The values of r(0) span a wide range, 10(6.5) <= r(0) <= 10(9.5) cm, with a mean value of < r(0)> similar to 10(8) cm. This is higher than the gravitational radius of a 10 M-circle dot black hole by a factor of approximate to 30. We argue that this result provides indirect evidence for jet propagation inside a massive star, and suggests the existence of recollimation shocks that take place close to this radius.

Place, publisher, year, edition, pages
2015. Vol. 813, no 2, 127
Keyword [en]
gamma rays: stars, hydrodynamics, methods: data analysis, radiation mechanisms: thermal, radiative transfer
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:su:diva-124764DOI: 10.1088/0004-637X/813/2/127ISI: 000365288900047OAI: oai:DiVA.org:su-124764DiVA: diva2:891886
Available from: 2016-01-08 Created: 2016-01-04 Last updated: 2016-01-08Bibliographically approved

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