Remnants from Gamma-Ray Bursts

Preprint
Publisher Website
Google Scholar
  • 8 November 2000
Abstract
We model the late time evolution of a gamma-ray burst by two blobs of matter colliding with the inter stellar medium. We follow the hydrodynamical evolution of this system numerically. We calculate the image of the remnant produced by bremsstrahlung and by synchrotron emission. We compare our results to DEM L 316, an object consisting of twin expanding shells. Our results can be rescaled to fit a variety of initial energies an so may be also applicable to other non-spherical remnants.

This publication has 0 references indexed in Scilit: