Computer Science
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..526..599k&link_type=abstract
GAMMA-RAY BURSTS: 5th Huntsville Symposium. AIP Conference Proceedings, Volume 526, pp. 599-602 (2000).
Computer Science
Jets And Bursts, Galactic Winds And Fountains, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Gamma-Ray Sources, Gamma-Ray Bursts
Scientific paper
The gamma ray burst (GRB) is the electric explosion of a rest-star from a white dwarf in our Galactic arm. The GRB destroys all white dwarfs before they could be red. This is the first publication of a new model which is proven by known measured emissions of the GRBs compared with the emissions of the solar flares. The new model explains not only the gamma rays, their short pulses, the later peaks of continuous and redshifted afterglows, the emission of relativistic protons, the non-thermal radiation, the deficit of weak bursts (as usual goals of GRB models), but also a so far un-revealed deficit of strong GRBs and the missing cold (red) white dwarfs. .
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