Detection of a Thermal Spectral Component in the Prompt Emission of GRB 100724B

Observations of GRB 100724B with the Fermi Gamma-Ray Burst Monitor (GBM) find that the spectrum is dominated by the typical Band functional form, which is usually taken to represent a non-thermal emission component, but also includes a statistically highly significant thermal spectral contribution....

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Veröffentlicht in:arXiv.org 2010-11
Hauptverfasser: Guiriec, Sylvain, Connaughton, Valerie, Briggs, Michael S, Burgess, Michael, Ryde, Felix, Daigne, Frédéric, Mészáros, Peter, Goldstein, Adam, McEnery, Julie, Omodei, Nicola, Bhat, P N, Bissaldi, Elisabetta, Camero-Arranz, Ascensión, Chaplin, Vandiver, Diehl, Roland, Fishman, Gerald, Foley, Suzanne, Gibby, Melissa, Giles, Misty M, Greiner, Jochen, Gruber, David, Andreas von Kienlin, Kippen, Marc, Kouveliotou, Chryssa, McBreen, Sheila, Meegan, Charles A, Paciesas, William, Preece, Robert, Rau, Arne, Tierney, Dave, Alexander J van der Horst, Wilson-Hodge, Colleen
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container_title arXiv.org
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creator Guiriec, Sylvain
Connaughton, Valerie
Briggs, Michael S
Burgess, Michael
Ryde, Felix
Daigne, Frédéric
Mészáros, Peter
Goldstein, Adam
McEnery, Julie
Omodei, Nicola
Bhat, P N
Bissaldi, Elisabetta
Camero-Arranz, Ascensión
Chaplin, Vandiver
Diehl, Roland
Fishman, Gerald
Foley, Suzanne
Gibby, Melissa
Giles, Misty M
Greiner, Jochen
Gruber, David
Andreas von Kienlin
Kippen, Marc
Kouveliotou, Chryssa
McBreen, Sheila
Meegan, Charles A
Paciesas, William
Preece, Robert
Rau, Arne
Tierney, Dave
Alexander J van der Horst
Wilson-Hodge, Colleen
description Observations of GRB 100724B with the Fermi Gamma-Ray Burst Monitor (GBM) find that the spectrum is dominated by the typical Band functional form, which is usually taken to represent a non-thermal emission component, but also includes a statistically highly significant thermal spectral contribution. The simultaneous observation of the thermal and non-thermal components allows us to confidently identify the two emission components. The fact that these seem to vary independently favors the idea that the thermal component is of photospheric origin while the dominant non-thermal emission occurs at larger radii. Our results imply either a very high efficiency for the non-thermal process, or a very small size of the region at the base of the flow, both quite challenging for the standard fireball model. These problems are resolved if the jet is initially highly magnetized and has a substantial Poynting flux.
doi_str_mv 10.48550/arxiv.1010.4601
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subjects Gamma ray bursts
Gamma rays
Photosphere
Physics - Cosmology and Nongalactic Astrophysics
Physics - High Energy Astrophysical Phenomena
Thermal emission
title Detection of a Thermal Spectral Component in the Prompt Emission of GRB 100724B
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