dc.contributor.author | GOROSABEL, J. | |
dc.contributor.author | RACUSIN, J. L. | |
dc.contributor.author | Page, M. J. | |
dc.contributor.author | De Pasquale, Massımılıano | |
dc.contributor.author | CASTRO-TIRADO, A. J. | |
dc.contributor.author | Smith, P. J. | |
dc.contributor.author | Breeveld, A. A. | |
dc.contributor.author | Kuin, N. P. M. | |
dc.contributor.author | Oates, S. R. | |
dc.date.accessioned | 2021-03-05T09:10:07Z | |
dc.date.available | 2021-03-05T09:10:07Z | |
dc.date.issued | 2015 | |
dc.identifier.citation | Oates S. R. , RACUSIN J. L. , De Pasquale M., Page M. J. , CASTRO-TIRADO A. J. , GOROSABEL J., Smith P. J. , Breeveld A. A. , Kuin N. P. M. , "Exploring the canonical behaviour of long gamma-ray bursts using an intrinsic multiwavelength afterglow correlation", MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.453, ss.4121-4135, 2015 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.other | vv_1032021 | |
dc.identifier.other | av_9ca05439-ca02-40ba-ab9b-221c08ac2846 | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/105237 | |
dc.identifier.uri | https://doi.org/10.1093/mnras/stv1956 | |
dc.description.abstract | In this paper, we further investigate the relationship, reported by Oates et al., between the optical/UV afterglow luminosity (measured at restframe 200 s) and average afterglow decay rate (measured from restframe 200 s onwards) of long duration gamma-ray bursts (GRBs). We extend the analysis by examining the X-ray light curves, finding a consistent correlation. We therefore explore how the parameters of these correlations relate to the prompt emission phase and, using a Monte Carlo simulation, explore whether these correlations are consistent with predictions of the standard afterglow model. We find significant correlations between: log L-O,L- 200 s and log L-X,L- 200 (s); alpha(O,> 200) (s) and alpha(X,> 200) (s), consistent with simulations. The model also predicts relationships between log E-iso and log L-200 (s); however, while we find such relationships in the observed sample, the slope of the linear regression is shallower than that simulated and inconsistent at greater than or similar to 3 sigma. Simulations also do not agree with correlations observed between log L-200 (s) and alpha(>200) (s), or log E-iso and alpha(>200) (s). Overall, these observed correlations are consistent with a common underlying physical mechanism producing GRBs and their afterglows regardless of their detailed temporal behaviour. However, a basic afterglow model has difficulty explaining all the observed correlations. This leads us to briefly discuss alternative more complex models. | |
dc.language.iso | eng | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | Temel Bilimler | |
dc.subject | Astronomi ve Astrofizik | |
dc.subject | ASTRONOMİ VE ASTROFİZİK | |
dc.subject | Uzay bilimi | |
dc.subject | Fizik | |
dc.title | Exploring the canonical behaviour of long gamma-ray bursts using an intrinsic multiwavelength afterglow correlation | |
dc.type | Makale | |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | |
dc.contributor.department | University Of London , , | |
dc.identifier.volume | 453 | |
dc.identifier.issue | 4 | |
dc.identifier.startpage | 4121 | |
dc.identifier.endpage | 4135 | |
dc.contributor.firstauthorID | 103550 | |