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Interpreting the kinematics of the extended gas in distant radiogalaxies from 8-10 m telescope spectra
2000
Astronomy and Astrophysics Supplement Series
The nature of the extreme kinematics in the extended gas of distant radio galaxies (z>0.7) is still an open question. With the advent of the 8-10 m telescope generation and the development of NIR arrays we are in the position for the first time to develop a more detailed study by using lines other than Lya and [OII]3727 depending on redshift. In this paper we review the main sources of uncertainty in the interpretation of the emission line kinematics: the presence of several kinematic
doi:10.1051/aas:2000303
fatcat:quqkai7k7vc35fvuahbj2iqhnq