Torus feeding and outflow launching in the active nucleus of the Circinus galaxy

Context. Most active galactic nuclei (AGNs) are believed to be surrounded by a dusty molecular torus on the parsec scale, which is often embedded within a larger circumnuclear disc (CND). Active galactic nuclei are fuelled by the inward transport of material through these structures and can launch multi-phase outflows that influence the host galaxy through AGN feedback. Aims. We use the Circinus galaxy as a nearby laboratory to investigate the physical mechanisms responsible for feeding the torus and launching a multi-phase outflow in this Seyfert-type AGN, as these mechanisms remain poorly understood. Methods. We analysed observations from the Atacama Large Millimeter/submillimeter Array of the Circinus nucleus at angular resolutions down to 13 mas (0.25 pc). We traced dust and the ionised outflow using 86 − 665 GHz continuum emission and studied the morphology and kinematics of the molecular gas using the HCO + (3-2), HCO + (4-3), HCN(3-2), HCN(4-3), and CO(3-2) transitions. Results. We find that the Circinus CND hosts molecular and dusty spiral arms, two of which connect directly to the torus. We detect inward mass transport along these structures and argue that the non-axisymmetric potential generated by these arms is the mechanism responsible for fuelling the torus. We estimate a feeding rate of 0.3 − 7.5 M ⊙ yr −1 , implying that over 88% of the inflowing material is expelled in a multi-phase outflow before reaching the accretion disc. The inferred feeding timescale ( t feed, torus = 120 kyr − 2.7 Myr) suggests that variability in AGN activity may be driven by changes in torus feeding. On parsec scales, the ionised outflow is traced by optically thin free-free emission. The outflow is stratified, with a slightly wider opening angle in the molecular phase than in the dusty and ionised components. The ionised outflow is launched or collimated by a warped accretion disc at a radius of r ∼ 0.16 pc, and its geometry requires an anisotropic launching mechanism.

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Journal
Astronomy and Astrophysics
Published
2025-10-20
DOI
https://doi.org/10.1051/0004-6361/202555556
Primary Topic
Plant Molecular Biology Research
Type
article
Field-Weighted Citation Impact
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article

Torus feeding and outflow launching in the active nucleus of the Circinus galaxy

A. P. S. Hygate, K. R. W. Tristram, C. M. Violette Impellizzeri, Sophie Venselaar et al.
Astronomy and Astrophysics
Plant Molecular Biology Research
article

Torus feeding and outflow launching in the active nucleus of the Circinus galaxy

A. P. S. Hygate, K. R. W. Tristram, C. M. Violette Impellizzeri, Sophie Venselaar, Wout M. Goesaert, Junzhi Wang 王均智, Zhiyu Zhang 张智昱
article en

Abstract

Context. Most active galactic nuclei (AGNs) are believed to be surrounded by a dusty molecular torus on the parsec scale, which is often embedded within a larger circumnuclear disc (CND). Active galactic nuclei are fuelled by the inward transport of material through these structures and can launch multi-phase outflows that influence the host galaxy through AGN feedback. Aims. We use the Circinus galaxy as a nearby laboratory to investigate the physical mechanisms responsible for feeding the torus and launching a multi-phase outflow in this Seyfert-type AGN, as these mechanisms remain poorly understood. Methods. We analysed observations from the Atacama Large Millimeter/submillimeter Array of the Circinus nucleus at angular resolutions down to 13 mas (0.25 pc). We traced dust and the ionised outflow using 86 − 665 GHz continuum emission and studied the morphology and kinematics of the molecular gas using the HCO + (3-2), HCO + (4-3), HCN(3-2), HCN(4-3), and CO(3-2) transitions. Results. We find that the Circinus CND hosts molecular and dusty spiral arms, two of which connect directly to the torus. We detect inward mass transport along these structures and argue that the non-axisymmetric potential generated by these arms is the mechanism responsible for fuelling the torus. We estimate a feeding rate of 0.3 − 7.5 M ⊙ yr −1 , implying that over 88% of the inflowing material is expelled in a multi-phase outflow before reaching the accretion disc. The inferred feeding timescale ( t feed, torus = 120 kyr − 2.7 Myr) suggests that variability in AGN activity may be driven by changes in torus feeding. On parsec scales, the ionised outflow is traced by optically thin free-free emission. The outflow is stratified, with a slightly wider opening angle in the molecular phase than in the dusty and ionised components. The ionised outflow is launched or collimated by a warped accretion disc at a radius of r ∼ 0.16 pc, and its geometry requires an anisotropic launching mechanism.

Astronomy and AstrophysicsVol. 704
Leiden University (NL), Ministry of Education (CL), Instituto de Estudios Universitarios (MX), Astronomy and Space (AU), Leiden Observatory, Nanjing University (CN), Universidad Diego Portales (CL), Netherlands Institute for Radio Astronomy (NL)
Openalex Percentile: Top 78%
Plant Molecular Biology Research
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