Titlebook: Radio Recombination Lines; Proceedings of a Wor P. A. Shaver Conference proceedings 1980 D. Reidel Publishing Company, Dordrecht, Holland 1

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Carbon Radio Recombination Line Emission from Dark CloudsSuch CII regions detectable by their radio recombination line radiation share several characteristics: they are all excited by.an early B-type star that is embedded within or closely associated with a dense (n k, 10. cm.) neutral cloud; the exciting star is identifiable both as a near infrared point

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The Galactic Center: Results of Radio Recombination Line Surveysned with a measurement of the continuum intensity, an estimate of the electron temperature of the source. In this chapter we will primarily be concerned with applying points (i) and (ii) to radio sources in the Galactic center.

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