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The active region in galactic nuclei: a spinar model
Shows that in the spinar model for active galactic nuclei the physical parameters of the central region are unequivocally determined by observational qualities. In homogeneous models the energy output via the inverse Compton effect should be of the same order as the primary emission. (5 refs).
| Autores principales: | , |
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| Lenguaje: | eng |
| Publicado: |
1978
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| Acceso en línea: | https://dx.doi.org/10.1086/182802 http://cds.cern.ch/record/879084 |