Hostname: page-component-7c8c6479df-fqc5m Total loading time: 0 Render date: 2024-03-29T00:06:29.431Z Has data issue: false hasContentIssue false

3-D TIGER Observations of Radio Galaxies

Published online by Cambridge University Press:  12 April 2016

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Copyright
Copyright © Astronomical Society of the Pacific 1997