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astro-ph1999
A model for the spatial distribution of relativistic electrons in the Crab Nebula
E. Amato, M. Salvati, R. Bandiera +2
We extend Pacini & Salvati's model for the synchrotron emission from plerions to allow more realistic predictions of the surface brightness profiles of the Crab Nebula at radio, op…
astro-ph1999
Beyond the standard model for the cosmic X-ray background
R. Gilli, G. Risaliti, M. Salvati
The synthesis model for the cosmic X-ray background (XRB) -based on the integrated emission of Active Galactic Nuclei (AGNs)- is complemented with new observational results. We ado…