Optical variability of the nuclei of the active galaxies NGC 3516 and 4151

Details Optical variability of the nuclei of the active galaxies NGC 3516 and 4151 Optical variability of the nuclei of the active galaxies NGC 3516 and 4151

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997kfnt...13c..78g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 13, p. 78, 79

Computer Science

Seyfert Galaxies, Active Galactic Nuclei, Ubv Spectra, Brightness Distribution, Light Curve, Compact Galaxies, Variability, Optical Properties

Scientific paper

New data on rapid UBVR variability of the nucleus of Seyfert galaxy NGC
3516 are obtained (9/10 May 1989). The amplitudes of brightness
variations are 0.09, 0.05, 0.07, and 0.05 m in U, B, V, and R,
respectively. The brightness variations of the nucleus of the galaxy NGC
4151 did not exceed 0.02 m in the course of the observations (3 h 08 m).

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