Optical monitoring of the Seyfert galaxy NGC 4151 and possible periodicities in its historical light curve
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1674-4527/14/i=8/a=003/pdf
Reference54 articles.
1. On the possible stellar origin of the optical variability of NGC 4151
2. THE FIRST SPECTROSCOPICALLY RESOLVED SUB-PARSEC ORBIT OF A SUPERMASSIVE BINARY BLACK HOLE
3. The Incidence of the Host Galaxy in Microvariability Observations of Quasars
4. CURVATURE OF THE SPECTRAL ENERGY DISTRIBUTIONS OF BLAZARS
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2. Broad-line region in NGC 4151 monitored by two decades of reverberation mapping campaigns – I. Evolution of structure and kinematics;Monthly Notices of the Royal Astronomical Society;2023-01-10
3. Possible mechanism for multiple changing-look phenomena in active galactic nuclei;Astronomy & Astrophysics;2020-09
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5. The Relative Wavelength Independence of IR Time Lags in NGC 4151 during the Years 2010–2015;Astronomy Letters;2019-04
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