Variability of emission lines in Seyfert-galaxy nuclei and quasars

Details Variability of emission lines in Seyfert-galaxy nuclei and quasars Variability of emission lines in Seyfert-galaxy nuclei and quasars

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sval....1...51b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 1, Mar. 1975, p. 12-17.) Soviet Astronomy Letters, vol. 1, Mar.-Apr. 1975, p. 51-53. Tr

Astronomy and Astrophysics

Astronomy

3

Emission Spectra, Galactic Nuclei, Line Spectra, Quasars, Seyfert Galaxies, X Ray Astronomy, Galactic Radiation, Gas Ionization, Ionizing Radiation, Optical Emission Spectroscopy

Scientific paper

As calculation shows, optical emission spectrum and emission line
variability of Seyfert galaxies and quasars nuclei can be explained by
heating and ionization of gas by variable 100-500 eV X-rays. The
required X-ray intensity agrees with observational data.

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