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Spectral Variability of Active Galactic Nuclei

Published online by Cambridge University Press:  21 February 2013

Y. L. Ai ,
W. Yuan  and
H. Y. Zhou
Y. L. Ai
Affiliation:
National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, China email: [email protected]
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
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Abstract

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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.

Keywords

Active galaxiesquasarsphotometric
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S290: Feeding Compact Objects: Accretion on All Scales , August 2012 , pp. 173 - 174
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