Changing-Look Narrow-Line Seyfert 1 Galaxies, their Detection with SVOM, and the Case of NGC 1566

Author:

Xu D. W.12,Komossa S.31,Grupe D.4ORCID,Wang J.51,Xin L. P.1,Han X. H.1,Wei J. Y.12,Bai J. Y.1,Bon E.6ORCID,Cangemi F.78,Cordier B.9,Dennefeld M.10,Gallo L. C.11,Kollatschny W.12,Kong De-Feng5,Ochmann M. W.1213,Qiu Y. L.1,Schartel N.14ORCID

Affiliation:

1. Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China

2. School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, China

3. Max–Planck Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany

4. Department of Physics, Geology, and Engineering Technology, Northern Kentucky University, 1 Nunn Drive, Highland Heights, KY 41099, USA

5. Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, Guangxi University, Nanning 530004, China

6. Astronomical Observatory Belgrade, Volgina 7, 11060 Belgrade, Serbia

7. Sorbonne Université, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies, LPNHE, 4 Place Jussieu, 75005 Paris, France

8. Université Paris-Cité, AstroParticules et Cosmologie, APC, 10 rue Alice Domon et Léonie Duquet, 75013 Paris, France

9. CEA-Saclay, IRFU/Departement d’Astrophysique, 91191 Gif-sur-Yvette, France

10. Institut d′Astrophysique de Paris, Sorbonne Université, CNRS, UMR 7095, 98 bis bd Arago, 75014 Paris, France

11. Department of Astronomy and Physics, Saint Mary’s University, 923 Robie Street, Halifax, NS B3H 3C3, Canada

12. Institut für Astrophysik und Geophysik, Universität Göttingen, Friedrich-Hund Platz 1, 37077 Göttingen, Germany

13. Ruhr University Bochum, Faculty of Physics and Astronomy, Astronomical Institute (AIRUB), 44780 Bochum, Germany

14. ESA, European Space Astronomy Centre (ESAC), Villanueva de la Cañada, E-28692 Madrid, Spain

Abstract

We discuss applications of the study of the new and barely explored class of changing-look (CL) narrow-line Seyfert 1 (NLS1) galaxies and comment on their detection with the space mission SVOM (Space Variable Objects Monitor). We highlight the case of NGC 1566, which is outstanding in many respects, for instance as one of the nearest known CL AGN undergoing exceptional outbursts. Its NLS1 nature is discussed, and we take it as a nearby prototype for systems that could be discovered and studied in the near future, including with SVOM. Finally, we briefly examine the broader implications and applications of CL events in NLS1 galaxies and show that such systems, once discovered in larger numbers, will greatly advance our understanding of the physics of the environment of rapidly growing supermassive black holes. This White Paper is part of a sequence of publications which explore aspects of our understanding of (CL) NLS1 galaxy physics with future missions.

Funder

National Natural Science Foundation of China

Serbian Ministry of Education, Science and Technological Development

German Aerospace Center (DLR) within the framework of the ‘Verbundforschung Astronomie und Astrophysik’

Publisher

MDPI AG

Subject

General Physics and Astronomy

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