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

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.

preprint1997arXivOpen access
Mark J. NeeserHans HippeleinKlaus Meisenheimer
astro-ph
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Open access3 authors1 topic
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Mark J. NeeserHans HippeleinKlaus Meisenheimer

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