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A Search for HI in Strong Radio Galaxies

Published online by Cambridge University Press:  25 May 2016

S. M. Simkin  and
J. Callcut
S. M. Simkin
Affiliation:
Michigan State University East Lansing, MI 48824-1116, USA
J. Callcut
Affiliation:
Michigan State University East Lansing, MI 48824-1116, USA

Extract

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In the past decade it has become clear that many classical, double radio galaxies have hosts with extensive ionized gas inside the body of the optical galaxy (Hansen et al., 1987) (Baum et al., 1988). We have observed three such sources (PKS349-27, PKS634-20, and Pictor A) in both Hα and HI (with the VLA).

Type
Properties of Radio Sources
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 183 - 184
Copyright
Copyright © Kluwer 1996 

References

Hansen, L., N≤rgaard-Nielsen, H.U., and J≤rgensen, H.E. (1987), A & A Sup. 71, pp. 465–491 Google Scholar
Baum, S.A., Heckman, T., Bridle, A., van Breughl, W. and Miley, G. (1988), Ap. J. Sup. 68, pp. 643–714 Google Scholar