Continuum reddening of Seyfert 1 nuclei

Details Continuum reddening of Seyfert 1 nuclei Continuum reddening of Seyfert 1 nuclei

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.204p..13c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 204, July 1983, p. 13P-18P. Research supported by Cambr

Astronomy and Astrophysics

Astronomy

21

Continuous Spectra, Galactic Nuclei, Interstellar Extinction, Seyfert Galaxies, Ubv Spectra, Emission Spectra, Interstellar Matter, Luminosity, Ultraviolet Absorption

Scientific paper

The authors show that the observed colours of Seyfert 1 nuclei are
tightly correlated with the inclination of the surrounding galaxies.
This allows to derive simple expressions giving the average reddening of
their continuum as a function of the axial ratio. The resulting values
of E(B-V) substantially exceed those for starlight.

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