The dust scattering model cannot explain the shallow X-ray decay in GRB afterglows (2009)

First Author: Shen R
Attributed to:  Swift Post-Launch Support at University of Leicester funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2008.14223.x

Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2008.14223.x

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2