The Coevolution of Galaxies and Supermassive Black Holes in the Near Universe



Título del documento: The Coevolution of Galaxies and Supermassive Black Holes in the Near Universe
Revista: Brazilian journal of physics
Base de datos: PERIÓDICA
Número de sistema: 000397480
ISSN: 0103-9733
Autores: 1
Instituciones: 1Universidade Federal do Rio Grande do Sul, Instituto de Fisica, Porto Alegre, Rio Grande do Sul. Brasil
Año:
Periodo: Dic
Volumen: 43
Número: 5-6
Paginación: 383-388
País: Brasil
Idioma: Inglés
Tipo de documento: Artículo
Enfoque: Analítico
Resumen en inglés A fundamental role is attributed to supermassive black holes (SMBH), and the feedback they generate, in the evolution of galaxies. But theoretical models trying to reproduce the MSMBH vs. sigma relation (between the SMBH mass and stellar velocity dispersion of the galaxy bulge) make broad assumptions about the physical processes involved. These assumptions are needed due to the scarcity of observational constraints on the relevant physical processes which occur when the SMBH is being fed via mass accretion in active galactic nuclei (AGN). In search for these constraints, our group—AGN integral field spectroscopy (AGNIFS)—has been mapping the gas kinematics as well as the stellar population properties of the inner few hundred parsecs of a sample of nearby AGN hosts. In this contribution, I report on results obtained so far which show gas inflows along nuclear spirals and compact disks in the inner tens to hundreds of pc in nearby AGN hosts which seem to be the sources of fuel to the AGN. As the inflow rates are much larger than the AGN accretion rate, the excess gas must be depleted via formation of new stars in the bulge. Indeed, in many cases, we find ∼100 pc circumnuclear rings of recent star formation (ages ∼10–500 Myr) that can be interpreted as a signature of coevolution of the host galaxy and its AGN. I also report on the mapping of outflows in ionized gas, which are ubiquitous in Seyfert galaxies, and discuss mass outflow rates and powers
Disciplinas: Física y astronomía
Palabras clave: Física,
Astrofísica,
Agujeros negros,
Galaxias,
Agujeros negros supermasivos,
Coevolución,
Núcleos activos galácticos,
Gases
Keyword: Physics and astronomy,
Physics,
Astrophysics,
Black holes,
Galaxies,
Supermassive black holes,
Coevolution,
Active galactic nuclei,
Gases
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