Hydrodynamic Properties of Gamma-Ray Burst Outflows Deduced from the Thermal Component

Citeable URL: https://ir.library.oregonstate.edu/concern/articles/fb494b07g

Descriptions

Attribute Name	Values
Creator	Pe'er, Asaf Barlow, Hugh O'Mahony, Shane Margutti, Raffaella Ryde, Felix Larsson, Josefin Lazzati, Davide Livio, Mario
Abstract	See article for Abstract. KEYWORDS: methods: data analysis, radiative transfer, radiation mechanisms: thermal, hydrodynamics, gamma rays: stars This is the publisher’s final pdf. The article is copyrighted by American Astronomical Society and published by IOP Publishing. It can be found at: http://iopscience.iop.org/article/10.1088/0004-637X/813/2127/meta;jsessionid=48B12A5B5CD563F9D995D5C936C31D3C.c2.iopscience.cld.iop.org
Resource Type	Article
DOI	https://doi.org/10.1088/0004-637X/813/2/127
Date Available	2016-01-12T17:14:26+00:00
Date Issued	2015-11-10
Citation	Pe’er, A., Barlow, H., O’Mahony, S., Margutti, R., Ryde, F., Larsson, J., ... & Livio, M. (2015). Hydrodynamic Properties of Gamma-Ray Burst Outflows Deduced from the Thermal Component. The Astrophysical Journal, 813(2), 127. doi:10.1088/0004-637X/813/2/127
Journal Title	The Astrophysical Journal
Journal Volume	813
Journal Issue/Number	2
Rights Statement	In Copyright
Funding Statement (additional comments about funding)	This research was partially supported by the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement no 618499. This work was supported in part by National Science Foundation grant No. PHYS-1066293.
Publisher	IOP Publishing
Peer Reviewed	Yes
Language	English [eng]
Replaces	http://hdl.handle.net/1957/58056