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Dust, H I and molecular gas must be important components of distant radio galaxies. Recent observations to detect these constituents are discussed.
McCarthy, P. J., Elston, R., and Eisenhardt, P.: 1992, ApJ387, L29.CrossRefGoogle Scholar
Miley, G. K.: 1994, in Bicknell, G. V., Dopita, M. A., and Quinn, P. J. (eds.), The First Stromlo Conference: The Physics of Active Galaxies, Vol. 54, p. 385.Google Scholar
Röttgering, H., Hunstead, R., Miley, G. K., van Ojik, R., and Wieringa, M. H.: 1994, Spatially Resolved Lyα Absorption in the z = 2.9 Radio Galaxy 0943–242, MN: submitted.Google Scholar
Solomon, P. M., Downes, D., and Radford, S. J. E.: 1992, ApJ398, L29.Google Scholar
Uson, J., Bagri, D. S., and Cornwell, D. S.: 1991, Phys. Rev. Letter67, 3328.Google Scholar
van Ojik, R., Röttgering, H., Miley, G., Bremer, M., Macchetto, F., and Chambers, K.: 1994, A&A289, 54.Google Scholar