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