Hostname: page-component-78c5997874-xbtfd Total loading time: 0 Render date: 2024-11-10T17:06:12.818Z Has data issue: false hasContentIssue false

Spectral Variability of Active Galactic Nuclei

Published online by Cambridge University Press:  21 February 2013

Y. L. Ai
Affiliation:
National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, China email: ayl@ynao.ac.cn
W. Yuan
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China
H. Y. Zhou
Affiliation:
Polar Research Institute of China, 451 Jinqiao Road, Pudong, Shanghai 200136, China
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

With SDSS multi-bands photometric data we propose that the variation of the nuclear continuum emission mostly accounts for the observed wavelength-dependent variability of active galactic nuclei.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013

References

Ai, Y. L., Yuan, W., Zhou, H. Y., Wang, T. G., Dong, X.-B., Wang, J. G., & Lu, H. L. 2010, ApJ, 716, 31CrossRefGoogle Scholar
Mannucci, F., et al. 2001, MNRAS, 326, 745Google Scholar
Vanden Berk, D. E., et al. 2001, AJ, 122, 549Google Scholar
Vanden Berk, D. E., et al. 2004, ApJ, 601, 692CrossRefGoogle Scholar
Zuo, Wenwen, Wu, Xue-Bing, Liu, Yi-Qing, Jiao, , & Cheng-Liang, 2012, arXiv:1209.0524Google Scholar