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3-D TIGER Observations of Radio Galaxies

Published online by Cambridge University Press:  12 April 2016

G. Adam ,
B. Rocca-Volmerange ,
P. Ferruit  and
R. Bacon
G. Adam
Affiliation:
CRAL, Observatoire de Lyon, F-69561 St. Genis Laval Cedex, France
B. Rocca-Volmerange
Affiliation:
IAP, CNRS, 98 bis Bd. Arago, F-75014 Paris, France
P. Ferruit
Affiliation:
CRAL, Observatoire de Lyon, F-69561 St. Genis Laval Cedex, France
R. Bacon
Affiliation:
CRAL, Observatoire de Lyon, F-69561 St. Genis Laval Cedex, France

Extract

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The cosmological evolution of stellar populations can be studied by observing, e.g,, high-z radio galaxies, and comparing their SEDs to those of local objects. But in such objects, the nuclear activity strongly influences the optical properties; to disentangle the superposition of spatial and spectral effects, complete 3-D data cubes are needed, such as those that can be obtained with the pioneering 3-D instrument TIGER.

Type
VI. The Narrow-Line Regions and Beyond
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 363 - 364
Copyright
Copyright © Astronomical Society of the Pacific 1997