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

Mark J. Neeser; Hans Hippelein; Klaus Meisenheimer

doi:10.1007/978-94-011-5238-9_4

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arXiv · astro-ph/9703038

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

Mark J. Neeser·Hans Hippelein·Klaus Meisenheimer

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Abstract

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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Mark J. Neeser, Hans Hippelein, Klaus Meisenheimer. 1997-03-06. Probing the Warm Gas in High Redshift Radio Galaxies: New Results on the Alignment Effect. https://doi.org/10.1007/978-94-011-5238-9_4

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