Abstract
The "canonical behavior" of the early X-ray afterglows of long-duration gamma-ray bursts (GRBs) - observed by the X-Ray Telescope of the Swift satellite - is precisely that predicted by the cannonball model of GRBs. © 2006. The American Astronomical Society. All rights reserved.
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CITATION STYLE
APA
Dado, S., Dar, A., & De Rújula, A. (2006). On the “Canonical Behavior” of the X-Ray Afterglows of Gamma-Ray Bursts Observed with Swift ’s XRT. The Astrophysical Journal, 646(1), L21–L24. https://doi.org/10.1086/506606
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