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dc.contributor.authorGranot, J.
dc.contributor.authorMiller, M.
dc.contributor.authorPiran, T.
dc.contributor.authorSuen, W.
dc.date.accessioned2011-11-07T12:01:08Z
dc.date.available2011-11-07T12:01:08Z
dc.date.issued2000
dc.identifier.citationGranot , J , Miller , M , Piran , T & Suen , W 2000 , Hydrodynamics and radiation from a relativistic expanding jet with applications to GRB afterglow . in Gamma-Ray Bursts : 5th Huntsville Symposium . AIP Conf Procs , vol. 526 , American Institute of Physics (AIP) , pp. 540-544 .
dc.identifier.otherPURE: 443395
dc.identifier.otherPURE UUID: 844d4609-e4d0-4f19-a9df-311d26c549e8
dc.identifier.otherdspace: 2299/1678
dc.identifier.urihttp://hdl.handle.net/2299/6926
dc.description.abstractWe describe fully relativistic three dimensional calculations of the slowing down and spreading of a relativistic jet by an external medium like the ISM. We calculate the synchrotron spectra and light curves using the conditions determined by the hydrodynamic calculations. Preliminary results with a moderate resolution are presented here. Higher resolution calculations are in progress.en
dc.language.isoeng
dc.publisherAmerican Institute of Physics (AIP)
dc.relation.ispartofGamma-Ray Bursts
dc.relation.ispartofseriesAIP Conf Procs
dc.titleHydrodynamics and radiation from a relativistic expanding jet with applications to GRB afterglowen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.versionAM
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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