The Optical Rebrightening of GRB100814A: An Interplay of Forward and Reverse Shocks?

Authors

M. De Pasquale, University College London Dorking
N.P.M. Kuin, University College London Dorking
S. Oates, University College London Dorking
S. Schulze, University of Iceland
Z. Cano, University of Iceland
C. Guidorzi, University of Ferrara
A. Beardmore, University of Leicester
P.A. Evans, University of Leicester
Z.L. Uhm, University of Nevada, Las Vegas
Bing Zhang, University of Nevada, Las VegasFollow
M. Page, University College London Dorking
S. Kobayashi, University of Leicester
A. Castro-Tirado, Instituto de Astrofísica de Andalucía
J. Gorosabel, Instituto de Astrofísica de Andalucía
T. Sakamoto, NASA Goddard Space Flight Center
T. Fatkhullin, Russian Academy of Science
S.B. Pandey, ARIES
M. Im, Seoul National University
P. Chandra, Pune University, Ganeshkhind
D. Frail, NRAO
H. Gao, University of Nevada, Las Vegas
D. Kopac, Liverpool John Moores University
Y. Jeon, Seoul National University
C. Akerlof, University of Michigan
K.Y. Huang, National Taiwan Normal University
S. Pak, Kyung Hee University
W.-K. Park, Seoul National University
A. Gomboc, University of Ljubljana
A. Melandri, INAF
S. Zane, University College London Dorking
C.G. Mundell, Liverpool John Moores University
C.J. Saxton, Israel Institute of Technology
S.T. Holland, Space Telescope Science Institute
F. Virgili, Astrophysics Research Institute, Liverpool
Y. Urata, National Central University, Cung-Li
I. Steele, Astrophysics Research Institute, Liverpool
D. Bersier, Astrophysics Research Institute, Liverpool
N. Tanvir, University of Leicester
V.V. Sokolov, Russian Academy of Sciences
A.S. Moskvitin, Russian Academy of Sciences

Document Type

Article

Publication Date

3-20-2015

Publication Title

Monthly Notices of the Royal Astronomical Society

Volume

449

Issue

1

First page number:

1024

Last page number:

1042

Abstract

We present a wide data set of gamma-ray, X-ray, UV/Opt/IR (UVOIR), and radio observations of the Swift GRB100814A. At the end of the slow decline phase of the X-ray and optical afterglow, this burst shows a sudden and prominent rebrightening in the optical band only, followed by a fast decay in both bands. The optical rebrightening also shows chromatic evolution. Such a puzzling behaviour cannot be explained by a single component model. We discuss other possible interpretations, and we find that a model that incorporates a long-lived reverse shock and forward shock fits the temporal and spectral properties of GRB100814 the best.

Keywords

Radiation mechanism: non-thermal; Shock waves; Gamma-ray burst: general

Disciplines

Astrophysics and Astronomy

File Format

pdf

File Size

1010 KB

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