The aim of this work is to understand the nature of the parent population of beamed narrow-line Seyfert 1 galaxies (NLS1s), by studying the physical properties of three parent candidates samples: steep-spectrum radio-loud NLS1s, radio-quiet NLS1s and disk-hosted radio-galaxies. In particular, we focused on the black hole mass and Eddington ratio distribution and on the interactions between the jet and the narrow-line region.

Exploring the parent population of beamed NLS1s: from the black hole to the jet

BERTON, MARCO;CIROI, STEFANO;CRACCO, VALENTINA;LA MURA, GIOVANNI;CONGIU, ENRICO;FREZZATO, MICHELE;RAFANELLI, PIERO
2015

Abstract

The aim of this work is to understand the nature of the parent population of beamed narrow-line Seyfert 1 galaxies (NLS1s), by studying the physical properties of three parent candidates samples: steep-spectrum radio-loud NLS1s, radio-quiet NLS1s and disk-hosted radio-galaxies. In particular, we focused on the black hole mass and Eddington ratio distribution and on the interactions between the jet and the narrow-line region.
High Energy Phenomena in Relativistic Outflows V
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/3221236
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