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

Germany); Hans Hippelein; Heidelberg; Klaus Meisenheimer (Max-Planck-Institut fuer Astronomie; Mark J. Neeser

arxiv: astro-ph/9703038 · v1 · pith:NAAUJ5S5new · submitted 1997-03-06 · 🌌 astro-ph

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

Mark J. Neeser , Hans Hippelein , Klaus Meisenheimer (Max-Planck-Institut fuer Astronomie , Heidelberg , Germany) This is my paper

classification 🌌 astro-ph

keywords radioalignmentgalaxiesresultswarmcreationdeptheffect

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

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