Abstract
The results discussed here are based on observations at λ 1 mm of 36 optically selected quasars (Sherwood et al., 1982; in preparation) and of 24 flat spectrum radio sources with Sν (5 GHz) ≥ 1 Jy (Kühr et al., 1979, 1981). H = 50 km/(s Mpc) and qo = 0 are used.
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Sherwood, W.A. (1983). QSO Luminosities at λ 1 MM. In: Abell, G.O., Chincarini, G. (eds) Early Evolution of the Universe and its Present Structure. International Astronomical Union / Union Astronomique Internationale, vol 104. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7220-9_13
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DOI: https://doi.org/10.1007/978-94-009-7220-9_13
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