The starburst model for the optical variability of the Seyfert 1 galaxies NGC 4151 and NGC 5548

Details The starburst model for the optical variability of the Seyfert 1 galaxies NGC 4151 and NGC 5548 The starburst model for the optical variability of the Seyfert 1 galaxies NGC 4151 and NGC 5548

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.205...69a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 205, no. 1, p. 69-76.

Astronomy and Astrophysics

Astrophysics

9

Astronomical Models, Seyfert Galaxies, Star Clusters, Starburst Galaxies, Light Curve, Metallicity

Scientific paper

The starburst model is used to show that the stellar processes expected to occur during the evolution of a metal-rich massive stellar cluster can reproduce the observed optical light curves of the Seyfert 1 NGC 4151 and NGC 5548. Observed supernovae can account for the energy and amplitude variations of individual peaks in the light curves of the nuclei. Numerical simulations under normal stellar evolution can reproduce the general shape of the light curves.

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