The MEGARA view of outflows in LINERs

Context. Feedback processes, in particular those driven by outflows, are believed to play a major role in galaxy evolution. Outflows are believed to be ubiquitous in all active galactic nuclei (AGNs), although their presence in low luminosity AGNs, in particular for Low-Ionisation Nuclear Emission l...

Descripción completa

Detalles Bibliográficos
Autores: Hermosa Muñoz, L., Cazzoli, S., Márquez, Isabel, Masegosa, Josefa, Gil de Paz, Armando, Castillo-Morales, A., Gallego, J., Carrasco, E., Iglesias-Páramo, J., García-Vargas, M. L., Gómez-Álvarez, P., Pascual, S., Pérez-Calpena, A., Cardiel, Nicolás
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2024
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/389136
Acceso en línea:http://hdl.handle.net/10261/389136
Access Level:acceso abierto
Palabra clave:Galaxies: active
Galaxies: ISM
Galaxies: kinematics and dynamics
Galaxies: nuclei
Galaxies: structure
Descripción
Sumario:Context. Feedback processes, in particular those driven by outflows, are believed to play a major role in galaxy evolution. Outflows are believed to be ubiquitous in all active galactic nuclei (AGNs), although their presence in low luminosity AGNs, in particular for Low-Ionisation Nuclear Emission line Regions (LINERs), has only started to be explored. Their properties (geometry, mass, and energetics) are still far from being properly characterised.

Similares en LA Referencia