Time Lag Between the Optical Continuum and Line Variabilities of NGC 4151

Details Time Lag Between the Optical Continuum and Line Variabilities of NGC 4151 Time Lag Between the Optical Continuum and Line Variabilities of NGC 4151

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..938...98k&link_type=abstract

SPECTRAL LINE SHAPES IN ASTROPHYSICS: VI Serbian Conference on Spectral Line Shapes in Astrophysics (VI SCSLSA). AIP Conference

Astronomy and Astrophysics

Astrophysics

Galactic Nuclei, Circumnuclear Matter, And Bulges

Scientific paper

Using a long term spectroscopic observation of NGC 4151 (obtained with 6
m telescope of SAO Russia, between 1996 and 2006) we used Z-Transfomed
Discrete Correlation Function (ZDCF) to find the time lag between the
broad Hβ and Hα lines and the optical continuum variably.

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