Light curve fittings of active galactic nuclei using supernova explosions

Details Light curve fittings of active galactic nuclei using supernova explosions Light curve fittings of active galactic nuclei using supernova explosions

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.171...61a&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astronomy

Active Galactic Nuclei, Astronomical Models, Light Curve, Supernovae, Accretion Disks, Black Holes (Astronomy), Interstellar Matter, Star Formation, Stellar Evolution, Supernova Remnants

Scientific paper

In the starburst-warmers scenario, a supernova (SN) explosion model was
used to construct theoretical light curves for active galactic nuclei.
The ionizing flux, in this model, should show variability according to
the SN rate in the galaxy.

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