High-resolution imaging of the multiphase AGN-driven outflow of NGC1068

Bibcode
2019hsax.conf..233V
Vives-Arias, H.; García-Burillo, S.; Ramos Almeida, C.
Referencia bibliográfica

Highlights on Spanish Astrophysics X, Proceedings of the XIII Scientific Meeting of the Spanish Astronomical Society held on July 16-20, 2018, in Salamanca, Spain, ISBN 978-84-09-09331-1. B. Montesinos, A. Asensio Ramos, F. Buitrago, R. Schödel, E. Villaver, S. Pérez-Hoyos, I. Ordóñez-Etxeberria (eds.) p. 233-233

Fecha de publicación:
3
2019
Número de autores
3
Número de autores del IAC
2
Número de citas
0
Número de citas referidas
0
Descripción
We analyze Atacama Large Millimeter Array (ALMA) observations of the CO(6-5) molecular line and the 432 μm continuum emission from the circumnuclear disk (CND) and the putative torus of the Seyfert 2 galaxy NGC 1068. The kinematics of both the CND and the torus show non-circular motions that are caused by outflows from the AGN. We compare the ALMA data with high-resolution near-infrared integral field spectroscopy of the molecular H_2 1-0S(1) line and some ionized species obtained with the VLT, and investigate the multiphase nature of the different ISM components of this prototypical AGN-driven outflow.
Tipo
Sin árbitro

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