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

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: steepspectrum radio-loud NLS1s, radio-quiet NLS1s and disk-hosted radiogalaxies. In particular, we focu...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Berton, Marco, Foschini, Luigi, Ciroi, Stefano, Caccianiga, Alessandro, Cracco, Valentina, La Mura, Giovanni, Di Mille, Francesco, Lister, Matthew, Mathur, Smita, Peterson, Bradley, J. L. Richards, Congiu, Enrico, Frezzato, Michele, Rafanelli, Piero
Formato: Objeto de conferencia
Lenguaje:Inglés
Publicado: 2015
Materias:
Ciencias Astronómicas
Seyfert 1 galaxies
black hole mass
Eddington ratio
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/167849
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
Descripción
Sumario: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: steepspectrum radio-loud NLS1s, radio-quiet NLS1s and disk-hosted radiogalaxies. In particular, we focused on the black hole mass and Eddington ratio distribution and on the interactions between the jet and the narrowline region.

Ejemplares similares