We present broadband observations and analysis of Swift gamma-ray burst (GRB)
120119A. Our early-time afterglow detections began under 15 s after the burst
in the host frame (redshift z = 1.73), and they yield constraints on the burst
energetics and local environment. Late-time afterglow observations of the burst
show evidence for a moderate column of dust (A_V ~ 1.1 mag) similar to, but
statistically distinct from, dust seen along Small Magellanic Cloud sightlines.
Deep late-time observations reveal a dusty, rapidly star-forming host galaxy.
Most notably, our early-time observations exhibit a significant red-to-blue
colour change in the first ~200 s after the trigger at levels heretofore unseen
in GRB afterglows. This colour change, which is coincident with the final
phases of the prompt emission, is a hallmark prediction of the photodestruction
of dust in GRB afterglows. We test whether dust-destruction signatures are
significantly distinct from other sources of colour change, namely a change in
the intrinsic spectral index \beta. We find that a time-varying power-law
spectrum alone cannot adequately describe the observed colour change, and
allowing for dust destruction (via a time-varying A_V) significantly improves
the fit. While not definitively ruling out other possibilities, this event
provides the best support yet for the direct detection of dust destruction in
the local environment of a GRB.
Description
[1305.1928] Evidence for Dust Destruction from the Early-time Colour Change of GRB 120119A
%0 Generic
%1 morgan2013evidence
%A Morgan, Adam N.
%A Perley, D. A.
%A Cenko, S. B.
%A Bloom, J. S.
%A Cucchiara, A.
%A Richards, J. W.
%A Filippenko, A. V.
%A Haislip, J. B.
%A LaCluyze, A.
%A Corsi, A.
%A Melandri, A.
%A Cobb, B. E.
%A Gomboc, A.
%A Horesh, A.
%A James, B.
%A Li, W.
%A Mundell, C. G.
%A Reichart, D. E.
%A Steele, I.
%D 2013
%K destruction dust grb
%T Evidence for Dust Destruction from the Early-time Colour Change of GRB
120119A
%U http://arxiv.org/abs/1305.1928
%X We present broadband observations and analysis of Swift gamma-ray burst (GRB)
120119A. Our early-time afterglow detections began under 15 s after the burst
in the host frame (redshift z = 1.73), and they yield constraints on the burst
energetics and local environment. Late-time afterglow observations of the burst
show evidence for a moderate column of dust (A_V ~ 1.1 mag) similar to, but
statistically distinct from, dust seen along Small Magellanic Cloud sightlines.
Deep late-time observations reveal a dusty, rapidly star-forming host galaxy.
Most notably, our early-time observations exhibit a significant red-to-blue
colour change in the first ~200 s after the trigger at levels heretofore unseen
in GRB afterglows. This colour change, which is coincident with the final
phases of the prompt emission, is a hallmark prediction of the photodestruction
of dust in GRB afterglows. We test whether dust-destruction signatures are
significantly distinct from other sources of colour change, namely a change in
the intrinsic spectral index \beta. We find that a time-varying power-law
spectrum alone cannot adequately describe the observed colour change, and
allowing for dust destruction (via a time-varying A_V) significantly improves
the fit. While not definitively ruling out other possibilities, this event
provides the best support yet for the direct detection of dust destruction in
the local environment of a GRB.
@misc{morgan2013evidence,
abstract = {We present broadband observations and analysis of Swift gamma-ray burst (GRB)
120119A. Our early-time afterglow detections began under 15 s after the burst
in the host frame (redshift z = 1.73), and they yield constraints on the burst
energetics and local environment. Late-time afterglow observations of the burst
show evidence for a moderate column of dust (A_V ~ 1.1 mag) similar to, but
statistically distinct from, dust seen along Small Magellanic Cloud sightlines.
Deep late-time observations reveal a dusty, rapidly star-forming host galaxy.
Most notably, our early-time observations exhibit a significant red-to-blue
colour change in the first ~200 s after the trigger at levels heretofore unseen
in GRB afterglows. This colour change, which is coincident with the final
phases of the prompt emission, is a hallmark prediction of the photodestruction
of dust in GRB afterglows. We test whether dust-destruction signatures are
significantly distinct from other sources of colour change, namely a change in
the intrinsic spectral index {\beta}. We find that a time-varying power-law
spectrum alone cannot adequately describe the observed colour change, and
allowing for dust destruction (via a time-varying A_V) significantly improves
the fit. While not definitively ruling out other possibilities, this event
provides the best support yet for the direct detection of dust destruction in
the local environment of a GRB.},
added-at = {2013-05-10T22:17:35.000+0200},
author = {Morgan, Adam N. and Perley, D. A. and Cenko, S. B. and Bloom, J. S. and Cucchiara, A. and Richards, J. W. and Filippenko, A. V. and Haislip, J. B. and LaCluyze, A. and Corsi, A. and Melandri, A. and Cobb, B. E. and Gomboc, A. and Horesh, A. and James, B. and Li, W. and Mundell, C. G. and Reichart, D. E. and Steele, I.},
biburl = {https://www.bibsonomy.org/bibtex/2a226f2ddfc157f430ee6a2b4fe28592f/miki},
description = {[1305.1928] Evidence for Dust Destruction from the Early-time Colour Change of GRB 120119A},
interhash = {9b7d4bfc7d609085a026393f09e3e678},
intrahash = {a226f2ddfc157f430ee6a2b4fe28592f},
keywords = {destruction dust grb},
note = {cite arxiv:1305.1928Comment: 15 pages, 11 figures; Submitted to MNRAS},
timestamp = {2013-05-10T22:17:36.000+0200},
title = {Evidence for Dust Destruction from the Early-time Colour Change of GRB
120119A},
url = {http://arxiv.org/abs/1305.1928},
year = 2013
}