Decoding the molecular torus of NGC 1068 Insights into its structure and kinematics from high-resolution ALMA observations

Context. Previous kinematic analysis of the pc-scale molecular torus in NGC 1068 have revealed a very complex and inhomogeneous system involving several physical components, such as non-circular motions, turbulence, high-velocity outflows, and possibly even counter-rotation.

Detalles Bibliográficos
Autores: Gámez Rosas, V., van der Werf, P., Gallimore, J. F., Impellizzeri, V., Jaffe, W., García-Burillo, Santiago, Aalto, S., Burtscher, L., Casasola, V., Combes, F., Henkel, C., Márquez, Isabel, Martín, S., Ramos Almeida, C., Viti, S., Fuente, A.
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:dnet:digitalcsic_::151ab8774a47193f27df330dc71c9da9
Acceso en línea:http://hdl.handle.net/10261/429160
Access Level:acceso abierto
Palabra clave:Molecular data
Galaxies: active
Galaxies: individual: NGC 1068
Galaxies: Seyfert
Descripción
Sumario:Context. Previous kinematic analysis of the pc-scale molecular torus in NGC 1068 have revealed a very complex and inhomogeneous system involving several physical components, such as non-circular motions, turbulence, high-velocity outflows, and possibly even counter-rotation.

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