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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

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