Cerenkov redshifts of Balmer lines in quasars

Details Cerenkov redshifts of Balmer lines in quasars Cerenkov redshifts of Balmer lines in quasars

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989scsmp..32..453c&link_type=abstract

Science in China, Series A - Mathematics, Physics, Astronomy and Technological Sciences (ISSN 0253-5831), vol. 32, April 1989, p

Mathematics

Logic

1

Astronomical Spectroscopy, Balmer Series, Cerenkov Radiation, Quasars, Red Shift, Active Galactic Nuclei, Doppler Effect, Forbidden Transitions, H I Regions, Lyman Alpha Radiation, Magnesium

Scientific paper

Estimates are given for the Cerenkov redshifts of Balmer lines in quasars and AGNs. It is found that the quasar high-ionization broad emission lines, such as C IV 1549 A, are blueshifted with respect to the neutral hydrogen and low-ionization broad bands. A line-emission mechanism, the Cerenkov line radiation (You et al., 1986) is used to explain broad emission lines of quasars.

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