A new mechanism for small redshift of H I broad lines with respect to C IV line in quasars

Details A new mechanism for small redshift of H I broad lines with respect to C IV line in quasars A new mechanism for small redshift of H I broad lines with respect to C IV line in quasars

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...358...18c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 358, July 20, 1990, p. 18-22. Research supported by the National Natural Sc

Astronomy and Astrophysics

Astrophysics

4

Active Galactic Nuclei, Emission Spectra, Galactic Radiation, Line Spectra, Quasars, Red Shift, Carbon, Cerenkov Radiation, H Lines

Scientific paper

Redshift differences in AGN are studied. The Cerenkov line redshift of the Balmer lines are calculated based on the Cerenkov line radiation theory, and the results are compared with observations. It is concluded that these redshifts provide an improved explanation for the fact that the high-ionization broad emission lines of quasars are blueshifted with respect to the H I and the low-ionization broad lines.

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