On the origin of the dramatic spectral variability of WPVS 007-Reference-Cited by-同舟云学术

On the origin of the dramatic spectral variability of WPVS 007

Published:2019-05-20 Issue:4 Volume:487 Page:4592-4602
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Li Junyao¹²^ORCID,Sun Mouyuan¹²^ORCID,Wang Tinggui¹²,He Zhicheng¹²,Xue Yongquan¹²

Affiliation:

1. CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, Anhui Province, China

2. School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, Anhui Province, China

Funder

NSFC

CAS Frontier Science Key Research Programme

China Postdoctoral Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1393/28675794/stz1393.pdf

Reference72 articles.

1. Compton heated winds and coronae above accretion disks. I Dynamics

2. A new powerful and highly variable disc wind in an AGN–star-forming galaxy, the case of MCG-03-58-007

3. SIMULATING THE TIMESCALE-DEPENDENT COLOR VARIATION IN QUASARS WITH A REVISED INHOMOGENEOUS DISK MODEL

4. EUCLIA—Exploring the UV/Optical Continuum Lag in Active Galactic Nuclei. I. A Model without Light Echoing

5. The Dust Content and Opacity of Actively Star‐forming Galaxies

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Investigating the Origin of the Absorption-line Variability in the Narrow-line Seyfert 1 Galaxy WPVS 007;The Astrophysical Journal;2023-08-01

2. Piercing through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields. II. Are Highly Obscured AGNs the Missing Link in the Merger-triggered AGN–Galaxy Coevolution Models?;The Astrophysical Journal;2020-10-30

3. Modeling Quasar UV/Optical Variability with the Corona-heated Accretion-disk Reprocessing (CHAR) Model;The Astrophysical Journal;2020-10-07