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A parsec-scale faint jet in the nearby changing-look Seyfert galaxy Mrk 590 | |
Yang, Jun1![]() ![]() | |
2021-03-01 | |
Source Publication | Monthly Notices of the Royal Astronomical Society
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ISSN | 0035-8711 |
Volume | 502Issue:1Pages:L61-L65 |
Contribution Rank | 10 |
Abstract | Broad Balmer emission lines in active galactic nuclei (AGN) may display dramatic changes in amplitude, even disappearance and re-appearance in some sources. As a nearby galaxy at a redshift of z = 0.0264, Mrk 590 suffered such a cycle of Seyfert type changes between 2006 and 2017. Over the last 50 yr, Mrk 590 also underwent a powerful continuum outburst and a slow fading from X-rays to radio wavelengths with a peak bolometric luminosity reaching about 10 per cent of the Eddington luminosity. To track its past accretion and ejection activity, we performed very long baseline interferometry (VLBI) observations with the European VLBI Network (EVN) at 1.6 GHz in 2015. The EVN observations reveal a faint (similar to 1.7 mJy) radio jet extending up to similar to 2.8 mas (projected scale similar to 1.4 pc) toward north, and probably resulting from the very intensive AGN activity. To date, such a parsec-scale jet is rarely seen in the known changing-look AGN. The finding of the faint jet provides further strong support for variable accretion as the origin of the type changes in Mrk 590. |
Keyword | galaxies: active galaxies: individual: Mrk 590 galaxies: jets galaxies: Seyfert radio continuum: galaxies active galactic nuclei observational evidence numerical-simulation radio observations accretion flows emission sample quasar evolution core Astronomy & Astrophysics |
Subtype | Article |
DOI | 10.1093/mnrasl/slab005 |
URL | 查看原文 |
Indexed By | SCI |
Language | 英语 |
WOS ID | WOS:000662142100012 |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/4724 |
Collection | 射电天文研究室_星系宇宙学研究团组 科研仪器设备产出_利用南山26米射电望远镜(NSRT)观测数据的文章 |
Corresponding Author | Yang, Jun |
Affiliation | 1.Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala, Sweden; 2.Joint Institute for VLBI ERIC (JIVE), Postbus 2, NL-7990 AA Dwingeloo, the Netherlands; 3.Max-Planck-Insitut f¨ur Radioastronomie, Auf dem H¨ugel 69, D-53121 Bonn, Germany; 4.Shanghai Astronomical Observatory, Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, 200030 Shanghai, China; 5.Institute of Astronomy and Astrophysics, Academia Sinica, Section 4, Roosevelt Rd., Taipei 10617, Taiwan; 6.CSIRO Astronomy and Space Science, Kensington 6151, Australia; 7.SURFsara, PO Box 94613, NL-1090 GP Amsterdam, the Netherlands; 8.Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands; 9.Netherlands Institute for Radio Astronomy (ASTRON), NL-7991 PD Dwingeloo, the Netherlands; 10.Xinjiang Astronomical Observatory, Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, 150 Science 1-Street, 830011 Urumqi, China; 11.Department of Astronomy, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, China |
Recommended Citation GB/T 7714 | Yang, Jun,van Bemmel, Ilse,Paragi, Zsolt,et al. A parsec-scale faint jet in the nearby changing-look Seyfert galaxy Mrk 590[J]. Monthly Notices of the Royal Astronomical Society,2021,502(1):L61-L65. |
APA | Yang, Jun.,van Bemmel, Ilse.,Paragi, Zsolt.,Komossa, S..,Yuan, Feng.,...&Wu, Qingwen.(2021).A parsec-scale faint jet in the nearby changing-look Seyfert galaxy Mrk 590.Monthly Notices of the Royal Astronomical Society,502(1),L61-L65. |
MLA | Yang, Jun,et al."A parsec-scale faint jet in the nearby changing-look Seyfert galaxy Mrk 590".Monthly Notices of the Royal Astronomical Society 502.1(2021):L61-L65. |
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