No CrossRef data available.
Article contents
Distant Radio Galaxies: the Strong Link between the Radio and Optical Emission
Published online by Cambridge University Press: 25 May 2016
Abstract
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.
Recent observations of distant radio galaxies show that there is a strong link between the radio source and the optical continuum and Lyα line emission from the galaxy. This link is discussed in terms of differences in age, orientation and environment between the radio sources.
- Type
- Cosmological Implications
- Information
- Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 583 - 584
- Copyright
- Copyright © Kluwer 1996
References
Best, P., Longair, M. S., Ruttgering, H. J. A., 1995, Evolution of the aligned structures in z ≃ 1 radio galaxies, MN: submitted
CrossRefGoogle Scholar
Ruttgering, H., Hunstead, R., Miley, G. K., van Ojik, R., Wieringa, M. H., 1995,
MNRAS
, 277, 389
CrossRefGoogle Scholar
van Ojik, R., Ruttgering, H., Carilli, C., Miley, G., Bremer, M., 1995a, A radio galaxy at z = 3.6 in a giant rotating Lyman α halo,
A&A
: in press
Google Scholar
van Ojik, R., Ruttgering, H. J. A., Miley, G. K., Hunstead, R., 1995b, The Gaseous Environment of Radio Galaxies in the Early Universe: Kinematics of the Lyman α Emission and Spatially Resolved HI Absorption,
A&A
: submitted
Google Scholar
You have
Access