The 3000 Å bump in quasars and Seyfert galaxies.

Details The 3000 Å bump in quasars and Seyfert galaxies. The 3000 Å bump in quasars and Seyfert galaxies.

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cha%26a..13..268m&link_type=abstract

Chin. Astron. Astrophys., Vol. 13, No. 3, p. 268 - 271

Astronomy and Astrophysics

Astrophysics

Radiation Mechanisms: Quasars, Radiation Mechanisms: Seyfert Galaxies

Scientific paper

The authors discuss the 3000 Å bump in quasars and Seyfert galaxies on the basis of the Cerenkov line emission model. They believe that the continuum around 3000 Å is made up of a nonthermal power-law spectrum, a black body spectrum from the accretion disk, a different black body spectrum from broad line region cloudlets and Fe II lines. Numerical calculation of the Seyfert galaxy NGC 4151 shows a good agreement with observations; it can be taken as a strong support for the Cerenkov line emission theory.

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