Correlation between the optical and X-ray variability of NGC 4151

Details Correlation between the optical and X-ray variability of NGC 4151 Correlation between the optical and X-ray variability of NGC 4151

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..496l&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, Nov. 1978, p. 496-499.) Soviet Astronomy Letters, vol. 4, Nov.-Dec. 1978, p. 267-269

Astronomy and Astrophysics

Astronomy

Seyfert Galaxies, X Ray Astronomy, Light Curve, Periodic Variations, Ubv Spectra

Scientific paper

A comparison of X-ray and optical observations of the variable Seyfert
galaxy during 1971-1976 reveals a correlation for both the slow and the
fast components of the light curves. The optical variability may lag
that in the X-ray range. The X-ray variability has a larger amplitude
and a shorter time scale.

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