dc.creator | De Pasquale, Massimiliano | |
dc.creator | Kuin, N. P. M. | |
dc.creator | Oates, S. | |
dc.creator | Schulze, S. | |
dc.creator | Cano, Z. | |
dc.creator | Guidorzi, C. | |
dc.creator | Beardmore, A. | |
dc.creator | Evans, P. A. | |
dc.creator | Uhm, Z. L. | |
dc.creator | Zhang, B. | |
dc.creator | Page, M. | |
dc.creator | Kobayashi, S. | |
dc.creator | Castro Tirado, A. | |
dc.creator | Gorosabel, J. | |
dc.creator | Sakamoto, T. | |
dc.creator | Fatkhullin, T. | |
dc.creator | Pandey, S. B. | |
dc.creator | Im, M. | |
dc.creator | Chandra, P. | |
dc.creator | Frail, D. | |
dc.creator | Gao, H. | |
dc.creator | Kopac, D. | |
dc.creator | Jeon, Y. | |
dc.creator | Akerlof, C. | |
dc.creator | Huang, K. Y. | |
dc.creator | Pak, S. | |
dc.creator | Park, W. K. | |
dc.creator | Gomboc, A. | |
dc.creator | Melandri, A. | |
dc.creator | Zane, S. | |
dc.creator | Mundell, C. G. | |
dc.creator | Saxton, C. J. | |
dc.creator | Holland, S. T. | |
dc.creator | Virgili, F. | |
dc.creator | Urata, Y. | |
dc.creator | Steele, I. | |
dc.creator | Bersier, D. | |
dc.creator | Tanvir, N. | |
dc.creator | Sokolov, V. V. | |
dc.creator | Moskvitin, A. S. | |
dc.date.accessioned | 2024-01-10T12:44:00Z | |
dc.date.accessioned | 2024-05-02T17:55:12Z | |
dc.date.available | 2024-01-10T12:44:00Z | |
dc.date.available | 2024-05-02T17:55:12Z | |
dc.date.created | 2024-01-10T12:44:00Z | |
dc.date.issued | 2015 | |
dc.identifier | 10.1093/mnras/stv267 | |
dc.identifier | 1365-2966 | |
dc.identifier | 0035-8711 | |
dc.identifier | https://doi.org/10.1093/mnras/stv267 | |
dc.identifier | https://repositorio.uc.cl/handle/11534/77639 | |
dc.identifier | WOS:000355345600074 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/9269344 | |
dc.description.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. | |
dc.language | en | |
dc.publisher | OXFORD UNIV PRESS | |
dc.rights | registro bibliográfico | |
dc.subject | radiation mechanism: non-thermal | |
dc.subject | shock waves | |
dc.subject | gamma-ray burst: general | |
dc.subject | GAMMA-RAY BURST | |
dc.subject | CONTINUOUS ENERGY INJECTION | |
dc.subject | AFTERGLOW LIGHT CURVES | |
dc.subject | SWIFT XRT DATA | |
dc.subject | X-RAY | |
dc.subject | BLAST WAVES | |
dc.subject | COMPREHENSIVE ANALYSIS | |
dc.subject | JET SIMULATIONS | |
dc.subject | GRB AFTERGLOWS | |
dc.subject | TELESCOPE | |
dc.title | The optical rebrightening of GRB100814A: an interplay of forward and reverse shocks? | |
dc.type | artículo | |