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Cited by 268

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Multiwavelength Afterglows in Gamma‐Ray Bursts: Refreshed Shock and Jet Effects

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Panaitescu, A., Meszaros, P., Rees, M. J.·1998·The Astrophysical Journal

Abstract

We present an analytical approach to calculate the hydrodynamics of the interaction between a relativistic ejecta and a surrounding medium, whose evolution serves as a model for gamma-ray burst (GRB) afterglows. We investigate the effect of the relevant model parameters on the X-ray, optical, and radio fluxes and the effect of a refreshed shock energy input and anisotropy in the ejecta on the shape of the light curves. We compare our numerical results to observed afterglows and give a quantitative description of the conditions (geometry and physical parameters) in the ejecta that are compatible with the light curves of the GRB 970508 afterglow, for which a large number of accurate flux measurements are available. We find that the radio, optical, and X-ray light curves of this afterglow can be explained satisfactorily within the spherically symmetric fireball model, assuming a delayed energy injection, or by an axially symmetric jet surrounded by a less energetic outflow.

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Metadata

Authors
Panaitescu, A., Meszaros, P., & Rees, M. J.
Venue
The Astrophysical Journal
Published
1998-08-10
Volume
503
Issue
1
Pages
314-324
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2169060213
Cited by
268
References
1
FWCI
15.11
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Multiwavelength Afterglows in Gamma‐Ray Bursts: Refreshed Shock and Jet Effects. https://app.cochat.ai/papers/10.1086/305995
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Panaitescu, A., Meszaros, P., & Rees, M. J. (1998). Multiwavelength Afterglows in Gamma‐Ray Bursts: Refreshed Shock and Jet Effects. The Astrophysical Journal. https://doi.org/10.1086/305995

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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