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A Detailed Study of High Redshift Radio Galaxies

Published online by Cambridge University Press:  12 April 2016

H. Hippelein ,
K. Meisenheimer  and
M. Neeser
H. Hippelein
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
K. Meisenheimer
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
M. Neeser
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany

Abstract

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We report on an ongoing survey of the extended line emission in high redshift radio galaxies, using a tunable Fabry-Perot etalon. Some results and suitable models are presented for individual sources.

Type
2. The Fabry-Perot Spectrometer and its Applications
Information
International Astronomical Union Colloquium , Volume 149: Tridimensional Optical Spectroscopic Methods in Astrophysics , 1995 , pp. 123 - 126
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Chambers, K.C., Miley, G.K., and van Breugel, W.J.M. 1987, Nature 329, 604 Google Scholar
Fosbury, R.A.E. 1985, in Structure and Evolution of Active Galactic Nuclei, 297.Google Scholar
Hippelein, H. and Meisenheimer, K. 1992, Astron. Astrophys. 264, 472 Google Scholar
LeFévre, O., Hammer, F., and Jones, J. 1988, ApJ 331, L73.Google Scholar
McCarthy, P.J., van Breugel, W.J.M., Spinrad, H., and Djorgovski, S. 1987, ApJ 321, L29.Google Scholar
Meisenheimer, K. and Hippelein, H. 1992, Astron. Astrophys. 264, 455 Google Scholar
Neeser, M., Hippelein, H. and Meisenheimer, K. 1994, in preparation.Google Scholar
van Breugel, W.J.M., Heckman, T.M., Miley, G.K., Filipenko, A.V. 1986, ApJ 311, 58.Google Scholar