A contemporaneous infrared flash from a long gamma-ray burst: an echo from the central engine
| dc.creator | Blake, C. H. | |
| dc.creator | Bloom, J. S. | |
| dc.creator | Starr, D. L. | |
| dc.creator | Falco, E. E. | |
| dc.creator | Skrutskie, M. | |
| dc.creator | Fenimore, E. E. | |
| dc.creator | Duchene, G. | |
| dc.creator | Szentgyorgyi, A. | |
| dc.creator | Hornstein, S. | |
| dc.creator | Prochaska, J. X. | |
| dc.creator | McCabe, C. | |
| dc.creator | Ghez, A. | |
| dc.creator | Konopacky, Q. | |
| dc.creator | Stapelfeldt, K. | |
| dc.creator | Hurley, K. | |
| dc.creator | Campbell, R. | |
| dc.creator | Kassis, M. | |
| dc.creator | Chaffee, F. | |
| dc.creator | Gehrels, N. | |
| dc.creator | Barthelmy, S. | |
| dc.creator | Cummings, J. R. | |
| dc.creator | Hullinger, D. | |
| dc.creator | Krimm, H. A. | |
| dc.creator | Markwardt, C. B. | |
| dc.creator | Palmer, D. | |
| dc.creator | Parsons, A. | |
| dc.creator | McLean, K. | |
| dc.creator | Tueller, J. | |
| dc.date | 2005-03-23 | |
| dc.date.accessioned | 2026-07-07T12:42:59Z | |
| dc.date.available | 2026-07-07T12:42:59Z | |
| dc.description | The explosion that results in a cosmic gamma-ray burst (GRB) is thought to produce emission from two physical processes -- the activity of the central engine gives rise to the high-energy emission of the burst through internal shocking and the subsequent interaction of the flow with the external environment produces long-wavelength afterglow. While afterglow observations continue to refine our understanding of GRB progenitors and relativistic shocks, gamma-ray observations alone have not yielded a clear picture of the origin of the prompt emission nor details of the central engine. Only one concurrent visible-light transient has been found and was associated with emission from an external shock. Here we report the discovery of infrared (IR) emission contemporaneous with a GRB, beginning 7.2 minutes after the onset of GRB 041219a. Our robotic telescope acquired 21 images during the active phase of the burst, yielding the earliest multi-colour observations of any long-wavelength emission associated with a GRB. Analysis of an initial IR pulse suggests an origin consistent with internal shocks. This opens a new possibility to study the central engine of GRBs with ground-based observations at long wavelengths. | |
| dc.description | Accepted to Nature on March 1, 2005. 9 pages, 4 figures, nature12.cls and nature1.cls files included. This paper is under press embargo until print publication | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0503508 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0503508 | |
| dc.identifier | Nature 435:181-184,2005 | |
| dc.identifier | doi:10.1038/nature03520 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/220269 | |
| dc.subject | Astrophysics | |
| dc.title | A contemporaneous infrared flash from a long gamma-ray burst: an echo from the central engine | |
| dc.type | text |