Abstract
Gamma-ray burst (GRB) afterglows are commonly interpreted as synchrotron emission from a relativistic blast wave produced by a point explosion in
Cite
CITATION STYLE
APA
Wang, X., & Loeb, A. (2000). Variability of Gamma‐Ray Burst Afterglows due to Interstellar Turbulence. The Astrophysical Journal, 535(2), 788–797. https://doi.org/10.1086/308888
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