A puzzle of radio-quiet quasar PG 1407 265: are optical and X-ray emissions produced from relativistic jet - Astrophysics > High Energy Astrophysical PhenomenaReportar como inadecuado




A puzzle of radio-quiet quasar PG 1407 265: are optical and X-ray emissions produced from relativistic jet - Astrophysics > High Energy Astrophysical Phenomena - Descarga este documento en PDF. Documentación en PDF para descargar gratis. Disponible también para leer online.

Abstract: PG 1407+265 is a radio quiet quasar but has a relativistic jet. In thisreport, we show some peculiar properties of its optical and X-ray emissions,which indicate their possible non-thermal origins produced from jet. We use asimple synchrotron + synchrotron self Compton SSC model to fit the emissionswith different ratios of energy densities between magnetic field and electrons\eta=UB-Ue, which predict different {\gamma}-ray luminosity. The First LATAGN Catalog 1LAC did not include PG 1407+265, which indicates an upper limitof {\gamma}-ray luminosity. This upper limit constrains the ratio unreasonablelarge \eta>10^4-10^5. This inversely indicates that the optical and X-rayemissions may be not produced from the beaming jet. We discuss the physicalimplications of these results.



Autor: Liang Chen, J. M. Bai

Fuente: https://arxiv.org/







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