Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8102
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dc.contributor.authorJoseph, P-
dc.contributor.authorGeorge, K-
dc.contributor.authorPaul, K. T-
dc.date.accessioned2023-01-05T06:29:06Z-
dc.date.available2023-01-05T06:29:06Z-
dc.date.issued2022-11-
dc.identifier.citationAstronomy and Astrophysics, Vol. 667, A88en_US
dc.identifier.issn1432-0746-
dc.identifier.urihttp://hdl.handle.net/2248/8102-
dc.descriptionOpen 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.abstractThe 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.isoenen_US
dc.publisherEDP Sciencesen_US
dc.relation.urihttps://doi.org/10.1051/0004-6361/202243923-
dc.rights© P. Joseph et al. 2022-
dc.subjectUltraviolet: galaxiesen_US
dc.subjectGalaxies: individual: NGC 3982en_US
dc.subjectGalaxies: activeen_US
dc.subjectGalaxies: star formationen_US
dc.titleActive galactic nucleus feedback in NGC 3982en_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

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