Physics
Scientific paper
Jan 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001iaus..205..150c&link_type=abstract
Galaxies and their Constituents at the Highest Angular Resolutions, Proceedings of IAU Symposium #205, held 15-18 August 2000 at
Physics
Scientific paper
We explore the relationship between extended radio and line emission for a radio-loud quasar sample including both core-dominated and lobe-dominated quasars. A strong correlation is present between extended radio and broad-line emission. The core emission is also correlated with the broad-line emission for the core-dominated quasars in the sample. The statistic behaviour on core emission of the lobe-dominated quasars is rather different from the core-dominated quasars. The extended radio luminosity is a good indicator for jet power, while the core luminosity can only be a jet power indicator for core-dominated quasars. The correlation between the ratio of Hβ to [O III] emission and ratio R of core to extended radio luminosity is investigated, which is in agreement with Jackson & Browne's (1991b) results. We further analyze the relation between the ratio of total broad-line to [O III] emission and find no evidence for anisotropy of broad-line emission.
Cao Xin-Wu
Jiang Dong Rong
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