Line profiles and continuum radiation in Seyfert galaxies

Details Line profiles and continuum radiation in Seyfert galaxies Line profiles and continuum radiation in Seyfert galaxies

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..549b&link_type=abstract

In ESA 3rd European IUE Conf. p 549-550 (SEE N83-11889 02-88)

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2

Continuous Radiation, Emission Spectra, Seyfert Galaxies, Ultraviolet Spectra, Continuums, Galactic Nuclei, Iue, Quasars, Resonance Lines

Scientific paper

The existence of general spectral properties common to all Seyfert 1 nuclei is considered. The IUE, and other UV data, indicate that in variable Seyfert nuclei the UV continuum is always harder when it is brighter. The full width at half maximum of CIII 1909 A is often found to be smaller than that of CIV 1550 A, in contrast with quasars where these lines appear with identical profiles.

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