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Two New Recombination-Line Results

Published online by Cambridge University Press:  14 August 2015

F. J. Kerr ,
P. D. Jackson ,
G. R. Knapp  and
R. L. Brown
F. J. Kerr
Affiliation:
University of Maryland, College Park, Md., U.S.A.
P. D. Jackson
Affiliation:
University of Maryland, College Park, Md., U.S.A.
G. R. Knapp
Affiliation:
University of Maryland, College Park, Md., U.S.A.
R. L. Brown
Affiliation:
National Radio Astronomy Observatory, Green Bank, W. Va., U.S.A.

Abstract

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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.

Type
Part 1: The Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 81 - 85
Copyright
Copyright © Reidel 1974 

References

Brown, R. L. and Knapp, G. R.: 1974, Astrophys. J. 189, 253.Google Scholar
Gordon, M. A.: 1973, Astrophys. J. 184, 77.Google Scholar
Gordon, M. A. and Gottesman, S. T.: 1971, Astrophys. J. 168, 361.Google Scholar
Gottesman, S. T. and Gordon, M. A.: 1970, Astrophys. J. Letters 162, L93.Google Scholar
Knapp, G. R.: 1972, Ph.D. thesis, University of Maryland.Google Scholar