Probing the Warm Gas in High Redshift Radio Galaxies: New Results on the Alignment Effect

Details Probing the Warm Gas in High Redshift Radio Galaxies: New Results on the Alignment Effect Probing the Warm Gas in High Redshift Radio Galaxies: New Results on the Alignment Effect

1997-03-06

arxiv.org/abs/astro-ph/9703038v1

Astronomy and Astrophysics

Astrophysics

6 pages, 2 postscript figures, uses crckapb10.sty and psfig.sty. To appear in "Observational Cosmology with the New Radio Surv

Scientific paper

We report on the results of an in depth investigation of the extended [OII]3727 line-emission in 11 3CR radio galaxies (0.5 < z < 1.1). Using a Fabry-Perot etalon to obtain both the kinematics and morphology of the [OII] gas, our goal was to find the mechanisms responsible for the creation and excitation of this warm gas, and the source of its alignment with the radio emission.

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