Detection of radio recombination-line emission from the rho OPH dark cloud.

1974 ◽  
Vol 189 ◽  
pp. 253 ◽  
Author(s):  
R. L. Brown ◽  
G. R. Knapp
1974 ◽  
Vol 192 ◽  
pp. 607 ◽  
Author(s):  
R. L. Brown ◽  
R. H. Gammon ◽  
G. R. Knapp ◽  
B. Balick

2018 ◽  
Vol 130 (990) ◽  
pp. 084101 ◽  
Author(s):  
Matteo Luisi ◽  
L. D. Anderson ◽  
T. M. Bania ◽  
Dana S. Balser ◽  
Trey V. Wenger ◽  
...  

1974 ◽  
Vol 60 ◽  
pp. 81-85
Author(s):  
F. J. Kerr ◽  
P. D. Jackson ◽  
G. R. Knapp ◽  
R. L. Brown

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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