Cerenkov redshift and the redshift difference among broad emission lines of quasars and active galactic nuclei
- 1 June 1989
- journal article
- Published by Elsevier in Physics Letters A
- Vol. 138 (4-5) , 165-167
- https://doi.org/10.1016/0375-9601(89)90020-0
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- New considerations on the broad-line regions of quasarsThe Astrophysical Journal, 1987
- Čerenkov line radiationPhysical Review A, 1986
- A new explanation of the Balmer decrement in quasarsPhysics Letters A, 1985
- Studies of broad emission line profiles in QSOs – I. Observed, high-resolution profilesMonthly Notices of the Royal Astronomical Society, 1984
- The Lyman-alpha emission-line profiles in high-redshift QSOsMonthly Notices of the Royal Astronomical Society, 1982
- A redshift difference between high and low ionization emission-line regions in QSOs - Evidence for radial motionsThe Astrophysical Journal, 1982
- Reverberation mapping of the emission line regions of Seyfert galaxies and quasarsThe Astrophysical Journal, 1982
- The emission lines of quasars and similar objectsReviews of Modern Physics, 1979
- The redshift difference between the broad and narrow emission lines in OQ 208Monthly Notices of the Royal Astronomical Society, 1979
- The Optical Spectrum of i Zwicky 1The Astrophysical Journal, 1976