Probing the Warm Gas in High Redshift Radio Galaxies: New Results on the Alignment Effect
arXiv:astro-ph/9703038 · doi:10.1007/978-94-011-5238-9_4
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.
6 pages, 2 postscript figures, uses crckapb10.sty and psfig.sty. To appear in "Observational Cosmology with the New Radio Surveys". Proc. of the Tenerife, Jan. 1997 Conference, ed. M. Bremer. Kluwer