Active galactic nucleus feedback in NGC 3982

Joseph, P; George, K; Paul, K. T

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dc.contributor.author	Joseph, P
dc.contributor.author	George, K
dc.contributor.author	Paul, K. T
dc.date.accessioned	2023-01-05T06:29:06Z
dc.date.available	2023-01-05T06:29:06Z
dc.date.issued	2022-11
dc.identifier.citation	Astronomy and Astrophysics, Vol. 667, A88	en_US
dc.identifier.issn	1432-0746
dc.identifier.uri	http://hdl.handle.net/2248/8102
dc.description	Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.	en_US
dc.description.abstract	The energetic feedback from supermassive black holes can influence star formation at the centres of galaxies. Observational evidence for active galactic nucleus (AGN) impact on star formation can be searched for in galaxies by combining ultraviolet imaging and optical integral field unit data. The ultraviolet flux directly traces recent star formation, and the integral field unit data can reveal dust attenuation, gas ionisation mechanisms, and gas kinematics from the central regions of the galaxy disk. A pilot study on NGC 3982 shows star formation suppression in the central regions of the galaxy, likely due to negative AGN feedback, and enhanced star formation in the outer regions. The case of NGC 3982 could be observational evidence of AGN feedback operating in a Seyfert galaxy.	en_US
dc.language.iso	en	en_US
dc.publisher	EDP Sciences	en_US
dc.relation.uri	https://doi.org/10.1051/0004-6361/202243923
dc.rights	© P. Joseph et al. 2022
dc.subject	Ultraviolet: galaxies	en_US
dc.subject	Galaxies: individual: NGC 3982	en_US
dc.subject	Galaxies: active	en_US
dc.subject	Galaxies: star formation	en_US
dc.title	Active galactic nucleus feedback in NGC 3982	en_US
dc.type	Article	en_US