Active galactic nucleus feedback in NGC 3982
- Title
- Active galactic nucleus feedback in NGC 3982
- Creator
- Joseph P.; George K.; Paul K.T.
- Description
- 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. 2022 EDP Sciences. All rights reserved.
- Source
- Astronomy and Astrophysics, Vol-667
- Date
- 2022-01-01
- Publisher
- EDP Sciences
- Subject
- Galaxies: Active; Galaxies: individual: NGC 3982; Galaxies: star formation; Ultraviolet: galaxies
- Coverage
- Joseph P., Department of Physics, CHRIST University, Bangalore, 560029, India, Indian Institute of Astrophysics, Bangalore, 560034, India; George K., Faculty of Physics, Ludwig-Maximilians-Universit, Scheinerstr. 1, Munich, 81679, Germany; Paul K.T., Department of Physics, CHRIST University, Bangalore, 560029, India
- Rights
- All Open Access; Green Open Access; Hybrid Gold Open Access
- Relation
- ISSN: 46361; CODEN: AAEJA
- Format
- Online
- Language
- English
- Type
- Article
Collection
Citation
Joseph P.; George K.; Paul K.T., “Active galactic nucleus feedback in NGC 3982,” CHRIST (Deemed To Be University) Institutional Repository, accessed February 26, 2025, https://archives.christuniversity.in/items/show/14863.