The origin of the prompt optical emission in GRB 060111B

G. Stratta; A. Pozanenko; J. L. Atteia; A. Klotz; S. Basa; B. Gendre; F. Verrecchia; M. Boer; S. Cutini; M. Henze; S. Holland; M. Ibrahimov; F. Ienna; I. Khamitov; S. Klose; V. Rumyantsev; V. Biryukov; F. Vachier; S. Arnouts; D. Perley

doi:10.1016/j.asr.2010.06.014

The origin of the prompt optical emission in GRB 060111B

G. Stratta, A. Pozanenko, J. L. Atteia, A. Klotz, S. Basa, B. Gendre, F. Verrecchia, M. Boer, S. Cutini, M. Henze, S. Holland, M. Ibrahimov, F. Ienna, I. Khamitov, S. Klose, V. Rumyantsev, V. Biryukov, F. Vachier, S. Arnouts, D. Perley

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Abstract

The detection of a bright optical emission measured with good temporal resolution during the prompt phase makes ORB 060111B a rare event that is especially useful for constraining theories of the prompt optical emission. Comparing this burst with other GRBs with evidence of optical peaks, we find that the optical peak epoch (t(p)) is anti-correlated with the high energy burst energetic assuming an isotropic energy release (E-iso) in agreement with Liang et al. (2009), and that the steeper is the post-peak afterglow decay, the less is the agreement with the correlation. GRB 060111B is among the tatters and it does not match the correlation. The Cannonball scenario is also discussed and we find that this model cannot be excluded for GRB 060111B. (C) 2010 COSPAR. Published by Elsevier Ltd. All rights reserved.

Original language	English
Pages (from-to)	1413-1415
Number of pages	3
Journal	Advances in Space Research
Volume	47
Issue number	8
DOIs	https://doi.org/10.1016/j.asr.2010.06.014
Publication status	Published - 15 Apr 2011
Externally published	Yes

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Stratta, G., Pozanenko, A., Atteia, J. L., Klotz, A., Basa, S., Gendre, B., Verrecchia, F., Boer, M., Cutini, S., Henze, M., Holland, S., Ibrahimov, M., Ienna, F., Khamitov, I., Klose, S., Rumyantsev, V., Biryukov, V., Vachier, F., Arnouts, S., & Perley, D. (2011). The origin of the prompt optical emission in GRB 060111B. Advances in Space Research, 47(8), 1413-1415. https://doi.org/10.1016/j.asr.2010.06.014

@article{1483b0e9c6664e82bb9f192f06da140b,

title = "The origin of the prompt optical emission in GRB 060111B",

abstract = "The detection of a bright optical emission measured with good temporal resolution during the prompt phase makes ORB 060111B a rare event that is especially useful for constraining theories of the prompt optical emission. Comparing this burst with other GRBs with evidence of optical peaks, we find that the optical peak epoch (t(p)) is anti-correlated with the high energy burst energetic assuming an isotropic energy release (E-iso) in agreement with Liang et al. (2009), and that the steeper is the post-peak afterglow decay, the less is the agreement with the correlation. GRB 060111B is among the tatters and it does not match the correlation. The Cannonball scenario is also discussed and we find that this model cannot be excluded for GRB 060111B. (C) 2010 COSPAR. Published by Elsevier Ltd. All rights reserved.",

keywords = "Gamma-ray burst, Non-thermal radiation, GAMMA-RAY BURSTS",

author = "G. Stratta and A. Pozanenko and Atteia, {J. L.} and A. Klotz and S. Basa and B. Gendre and F. Verrecchia and M. Boer and S. Cutini and M. Henze and S. Holland and M. Ibrahimov and F. Ienna and I. Khamitov and S. Klose and V. Rumyantsev and V. Biryukov and F. Vachier and S. Arnouts and D. Perley",

year = "2011",

month = apr,

day = "15",

doi = "10.1016/j.asr.2010.06.014",

language = "English",

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Stratta, G, Pozanenko, A, Atteia, JL, Klotz, A, Basa, S, Gendre, B, Verrecchia, F, Boer, M, Cutini, S, Henze, M, Holland, S, Ibrahimov, M, Ienna, F, Khamitov, I, Klose, S, Rumyantsev, V, Biryukov, V, Vachier, F, Arnouts, S & Perley, D 2011, 'The origin of the prompt optical emission in GRB 060111B', Advances in Space Research, vol. 47, no. 8, pp. 1413-1415. https://doi.org/10.1016/j.asr.2010.06.014

TY - JOUR

T1 - The origin of the prompt optical emission in GRB 060111B

AU - Stratta, G.

AU - Pozanenko, A.

AU - Atteia, J. L.

AU - Klotz, A.

AU - Basa, S.

AU - Gendre, B.

AU - Verrecchia, F.

AU - Boer, M.

AU - Cutini, S.

AU - Henze, M.

AU - Holland, S.

AU - Ibrahimov, M.

AU - Ienna, F.

AU - Khamitov, I.

AU - Klose, S.

AU - Rumyantsev, V.

AU - Biryukov, V.

AU - Vachier, F.

AU - Arnouts, S.

AU - Perley, D.

PY - 2011/4/15

Y1 - 2011/4/15

N2 - The detection of a bright optical emission measured with good temporal resolution during the prompt phase makes ORB 060111B a rare event that is especially useful for constraining theories of the prompt optical emission. Comparing this burst with other GRBs with evidence of optical peaks, we find that the optical peak epoch (t(p)) is anti-correlated with the high energy burst energetic assuming an isotropic energy release (E-iso) in agreement with Liang et al. (2009), and that the steeper is the post-peak afterglow decay, the less is the agreement with the correlation. GRB 060111B is among the tatters and it does not match the correlation. The Cannonball scenario is also discussed and we find that this model cannot be excluded for GRB 060111B. (C) 2010 COSPAR. Published by Elsevier Ltd. All rights reserved.

AB - The detection of a bright optical emission measured with good temporal resolution during the prompt phase makes ORB 060111B a rare event that is especially useful for constraining theories of the prompt optical emission. Comparing this burst with other GRBs with evidence of optical peaks, we find that the optical peak epoch (t(p)) is anti-correlated with the high energy burst energetic assuming an isotropic energy release (E-iso) in agreement with Liang et al. (2009), and that the steeper is the post-peak afterglow decay, the less is the agreement with the correlation. GRB 060111B is among the tatters and it does not match the correlation. The Cannonball scenario is also discussed and we find that this model cannot be excluded for GRB 060111B. (C) 2010 COSPAR. Published by Elsevier Ltd. All rights reserved.

KW - Gamma-ray burst

KW - Non-thermal radiation

KW - GAMMA-RAY BURSTS

U2 - 10.1016/j.asr.2010.06.014

DO - 10.1016/j.asr.2010.06.014

M3 - Article

SN - 0273-1177

VL - 47

SP - 1413

EP - 1415

JO - Advances in Space Research

JF - Advances in Space Research

IS - 8

ER -

The origin of the prompt optical emission in GRB 060111B

Abstract

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