MaNGA AGN dwarf galaxies (MAD): II. AGN outflows in dwarf galaxies

[Context] Feedback from an active galactic nucleus (AGN) is one of the most important mechanisms in galaxy evolution. This phenomenon is usually found in massive galaxies and is known to regulate star formation. Although dwarf galaxies are assumed to be regulated by supernova feedback, recent studie...

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Detalles Bibliográficos
Autores: Rodríguez Morales, Víctor, Mezcua, Mar, Domínguez Sánchez, Helena, Audibert, Anelise, Müller-Sánchez, Francisco, Siudek, Malgorzata, Eróstegui, Alejandro
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2025
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/398678
Acceso en línea:http://hdl.handle.net/10261/398678
http://arxiv.org/abs/2503.07779v2
Access Level:acceso abierto
Palabra clave:Galaxies: active
Galaxies: dwarf
Galaxy: evolution
Descripción
Sumario:[Context] Feedback from an active galactic nucleus (AGN) is one of the most important mechanisms in galaxy evolution. This phenomenon is usually found in massive galaxies and is known to regulate star formation. Although dwarf galaxies are assumed to be regulated by supernova feedback, recent studies have offered evidence to support the presence of AGN outflows and feedback in dwarf galaxies.

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