Krühler, T. 2009 GRB 080710的余辉观测
主要内容:
可能是一个偏轴的暴.
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Title: | The bright optical/NIR afterglow of the faint GRB 080710 - Evidence for a jet viewed off axis | |
Authors: | Krühler, T.; Greiner, J.; Afonso, P.; Burlon, D.; Clemens, C.; Filgas, R.; Kann, D. A.; Klose, S.; Küpcü Yoldas, A.; McBreen, S.; Olivares, F.; Rau, A.; Rossi, A.; Schulze, S.; Szokoly, G. P.; Updike, A.; Yoldas, A. | |
Publication: | eprint arXiv:0908.2250 | |
Publication Date: | 08/2009 | |
Origin: | ARXIV | |
Keywords: | Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Extragalactic Astrophysics | |
Comment: | 9 pages, 4 figures, accepted by A and A | |
Bibliographic Code: | 2009arXiv0908.2250K |
Abstract
We investigate the optical/near-infrared light curve of the afterglow of GRB 080710 in the context of rising afterglows. Optical and near-infrared photometry was performed using the seven channel imager GROND and the Tautenburg Schmidt telescope. X-ray data were provided by the X-ray Telescope onboard the Swift satellite. The optical/NIR light curve of the afterglow of GRB 080710 is dominated by an initial increase in brightness, which smoothly turns over into a shallow power law decay. The initially rising achromatic light curve of the afterglow of GRB 080710 can be accounted for with a model of a burst viewed off-axis or a single jet in its pre deceleration phase and in an on-axis geometry. An unified picture of the afterglow light curve and prompt emission properties can be obtained with an off-axis geometry, suggesting that late and shallow rising optical light curves of GRB afterglows might be produced by geometric effects.Bibtex entry for this abstract Preferred format for this abstract (see Preferences)
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