Abstract
This paper reports two new recombination-line results. The first is the detection of carbon line emission from the dark cloud near ϱ Ophiuchi, and the second discusses the origin of hydrogen recombination line emission associated with ionized gas outside known discrete continuum sources.
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Brown, R. L. and Knapp, G. R.: 1974, Astrophys. J.189, 253.
Gordon, M. A.: 1973, Astrophys. J.184, 77.
Gordon, M. A. and Gottesman, S. T.: 1971, Astrophys. J.168, 361.
Gottesman, S. T. and Gordon, M. A.: 1970, Astrophys. J. Letters 162, L93.
Knapp, G. R.: 1972, Ph.D. thesis, University of Maryland.
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Kerr, F.J., Jackson, P.D., Knapp, G.R., Brown, R.L. (1974). Two New Recombination-Line Results. In: Kerr, F.J., Simonson, S.C. (eds) Galactic Radio Astronomy. International Astronomical Union/ Union Astronomique Internationale, vol 60. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2263-7_7
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DOI: https://doi.org/10.1007/978-94-010-2263-7_7
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