Investigating the effects of fresh gas on the active galactic nuclei luminosity of early- and late-type galaxies
Investigating the effects of fresh gas on the active galactic nuclei luminosity of early- and late-type galaxies
The main fuelling processes for active galactic nuclei (AGN) are currently unknown. Previous work showed that galaxies with a large kinematic misalignment between their stellar and gas reservoirs have a higher AGN fraction than galaxies without misalignment. Such misalignment is a strong indication of a past galaxy interaction or an external accretion event. In this work, we use integral field spectroscopy data from the Sydney-Australian-Astronomical-Observatory Multi-object Integral-Field Spectrograph (SAMI) and the Mapping Nearby Galaxies at APO (MaNGA) surveys to investigate the AGN luminosity as a function of kinematic misalignment angle. Our sample of AGN exhibit bolometric luminosities in the range-erg s, indicative of low to moderate luminosity AGN. We find no correlation between AGN luminosity as a function of misalignment for AGN host galaxies from both surveys. We find some differences between the AGN luminosity of early-and late-Type AGN host galaxies (ETGs, LTGs). AGN in LTG hosts have a wider luminosity range, with most LTG hosts showing aligned stellar to gas kinematics. AGN in ETG hosts have a luminosity range that does not depend on misalignment angle, suggesting AGN in ETG hosts are consistent with being fuelled by external accretion events, irrespective of their stellar to gas kinematic misalignment. While all the AGN in ETGs in our sample are consistent with being activated and fuelled by external gas, the range of observed AGN luminosities is likely caused by secondary factors such as the amount of fresh gas brought into the galaxy by the external interaction.
galaxies: Active, galaxies: ISM, galaxies: nuclei, quasars: supermassive black holes
1191-1200
Winiarska, Martyna w
362f5de7-c10d-4109-a3e0-c4d65a44f50f
Raimundo, Sandra i
e409d9d3-17e8-4049-ad29-43ada60b24e2
Davis, Timothy a
3e695002-beb7-42f9-a10d-f8941bbde344
Riffel, Rogério
086a846f-4562-497a-9ee0-53eaee1d0066
Shankar, Francesco
b10c91e4-85cd-4394-a18a-d4f049fd9cdb
Wiseman, Phil
abd591bd-121f-4dc1-bfce-090f01432bb4
13 March 2025
Winiarska, Martyna w
362f5de7-c10d-4109-a3e0-c4d65a44f50f
Raimundo, Sandra i
e409d9d3-17e8-4049-ad29-43ada60b24e2
Davis, Timothy a
3e695002-beb7-42f9-a10d-f8941bbde344
Riffel, Rogério
086a846f-4562-497a-9ee0-53eaee1d0066
Shankar, Francesco
b10c91e4-85cd-4394-a18a-d4f049fd9cdb
Wiseman, Phil
abd591bd-121f-4dc1-bfce-090f01432bb4
Winiarska, Martyna w, Raimundo, Sandra i, Davis, Timothy a, Riffel, Rogério, Shankar, Francesco and Wiseman, Phil
(2025)
Investigating the effects of fresh gas on the active galactic nuclei luminosity of early- and late-type galaxies.
Monthly Notices Of The Royal Astronomical Society, 538 (2), .
(doi:10.1093/mnras/staf295).
Abstract
The main fuelling processes for active galactic nuclei (AGN) are currently unknown. Previous work showed that galaxies with a large kinematic misalignment between their stellar and gas reservoirs have a higher AGN fraction than galaxies without misalignment. Such misalignment is a strong indication of a past galaxy interaction or an external accretion event. In this work, we use integral field spectroscopy data from the Sydney-Australian-Astronomical-Observatory Multi-object Integral-Field Spectrograph (SAMI) and the Mapping Nearby Galaxies at APO (MaNGA) surveys to investigate the AGN luminosity as a function of kinematic misalignment angle. Our sample of AGN exhibit bolometric luminosities in the range-erg s, indicative of low to moderate luminosity AGN. We find no correlation between AGN luminosity as a function of misalignment for AGN host galaxies from both surveys. We find some differences between the AGN luminosity of early-and late-Type AGN host galaxies (ETGs, LTGs). AGN in LTG hosts have a wider luminosity range, with most LTG hosts showing aligned stellar to gas kinematics. AGN in ETG hosts have a luminosity range that does not depend on misalignment angle, suggesting AGN in ETG hosts are consistent with being fuelled by external accretion events, irrespective of their stellar to gas kinematic misalignment. While all the AGN in ETGs in our sample are consistent with being activated and fuelled by external gas, the range of observed AGN luminosities is likely caused by secondary factors such as the amount of fresh gas brought into the galaxy by the external interaction.
Text
2502.08715v1
- Author's Original
More information
Accepted/In Press date: 12 February 2025
e-pub ahead of print date: 18 February 2025
Published date: 13 March 2025
Keywords:
galaxies: Active, galaxies: ISM, galaxies: nuclei, quasars: supermassive black holes
Identifiers
Local EPrints ID: 501429
URI: http://eprints.soton.ac.uk/id/eprint/501429
ISSN: 1365-2966
PURE UUID: e3705c4b-1fb8-4cb2-80ed-cc1134330d8c
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Date deposited: 30 May 2025 16:59
Last modified: 20 Sep 2025 02:13
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Contributors
Author:
Martyna w Winiarska
Author:
Timothy a Davis
Author:
Rogério Riffel
Author:
Phil Wiseman
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