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19982003
most citedSuperluminal Motion and Relativistic Beaming in Blazar Jets

1 citations · 1 across the 3 of their papers we have counts for

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astro-ph2003

Variability and Velocity of Superluminal Sources

M. H. Cohen, M. A. Russo, D. C. Homan +5

We investigate the relation between the Doppler factor determined from variations in total flux at 22 and 37 GHz, and the apparent transverse velocity determined from VLBA observat…

astro-ph20021 cited

Superluminal Motion and Relativistic Beaming in Blazar Jets

K. I. Kellermann, M. L. Lister, D. C. Homan +5

High resolution radio observations remain the most direct way to study the formation and evolution of radio jets associated with the accretion onto massive black holes. We report p…

astro-ph2002

Kinematics of parsec-scale structures in AGN: the 2cm VLBA Survey

E. Ros, K. I. Kellermann, M. L. Lister +5

We are investigating the kinematics of jets in active galactic nuclei on parsec scales by studying a representative population of sources. This study is being carried out using the…

astro-ph1999

The NV/CIV ratio in high redshift radio galaxies

R. A. E. Fosbury, J. Vernet, M. Villar-Martin +3

Deep Keck spectropolarimetry has been obtained of a sample of powerful radio galaxies with . In addition to a clear 2200Ådust scattering/extinction signature and…

astro-ph1998

The structure and composition of high redshift radio galaxies

R A E Fosbury, J Vernet, M Villar-Martin +4

Keck spectropolarimetry, giving spectral coverage from Ly- to beyond CIII], and HST imaging of a sample of powerful radio galaxies with \ has been obtained. These data…

astro-ph1998

Optical continuum structure of Cygnus A

R. A. E. Fosbury, J. Vernet, M. Villar-Martin +4

As a prerequisite for interpreting new observations of the most distant radio galaxies, we make an optical study of the closest powerful radio source, Cygnus A. Using Keck imaging-…