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HI Imaging of Radio Active Ellipticals

Published online by Cambridge University Press:  04 August 2017

J.H. van Gorkom
J.H. van Gorkom*
Affiliation:
Princeton University Observatory, Peyton Hall, Princeton, NJ 08544, USA

Abstract

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Statistics on HI absorption in radio galaxies suggest that accretion of gas into the center might be a general phenomenon. Images of the HI emission from these galaxies show that the gas must have an external origin. The rotation curves derived from the HI data are flat.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 127: Structure and Dynamics of Elliptical Galaxies , 1987 , pp. 421 - 422
Copyright
Copyright © Reidel 1987 

References

REFERENCES

Knapp, G.R., 1987. This volume, p. 145.Google Scholar
van Gorkom, , Knapp, , Raimond, , Faber, , Gallagher, , 1986. A. J., 91, 791 CrossRefGoogle Scholar
van Gorkom, van der Hulst, Haschick, Tubbs, 1987. in preparation Google Scholar