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Gas Disks in Radio Galaxies

Published online by Cambridge University Press:  07 August 2017

S. M. Simkin  and
Elaine M. Sadler
S. M. Simkin
Affiliation:
Michigan State University
Elaine M. Sadler
Affiliation:
Anglo-Australian Observatory

Extract

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Spectroscopic observations have shown that strong radio galaxies contain extra–nuclear gas which is rapidly rotating (Simkin 1979, Heckman et al. 1985). In addition, weak spiral-like structure has been observed in the inner regions of several strong radio galaxies classified as DE or E (Simkin and Michel 1986, Beichman et al. 1985, Hansen et al. 1987, Baum et al. 1988).

Type
Part 8: Relationships of Nucleus, Galaxy and Environment
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 484 - 485
Copyright
Copyright © Kluwer 1989 

References

Baum, S.A. et al. 1988. Ap. J. Suppl., in press.Google Scholar
Beichman, C. et al. 1985. Ap. J. 293, 148.Google Scholar
Hansen, L., Norgaard–Nielsen, H.U., Jorgensen, H.E., 1987. Astr. Ap. Suppl. 71, 465.Google Scholar
Heckman, T.M., Illingworth, G.D., Miley, G.K. & van Breughel, W.J.M. 1985. Ap. J. 299, 41.CrossRefGoogle Scholar
Rubin, V.C., Burstein, D., Ford, W.K. & Thonnard, N. 1985. Ap. J. 289, 81.Google Scholar
Simkin, S.M. & Michel, A. 1986. Ap. J. 300, L5.CrossRefGoogle Scholar