Abstract
view Abstract Citations (19) References (8) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Classification of OH Radio Emission Sources Ball, John A. ; Staelin, David H. Abstract Those OH emission sources which emit most strongly at 1665 or 1667 MHz seem to be associated with H ii regions, whereas those OH emission sources which emit most strongly at 1720 or ~612 MHz seem to be associated with combinations of non-thermal radio sources and 11 ii regions. New observations at 1720 MHz are reported which indicate that the emission lines in those regions associated with non-thermal radio sources are less polarized Publication: The Astrophysical Journal Pub Date: July 1968 DOI: 10.1086/180216 Bibcode: 1968ApJ...153L..41B full text sources ADS |
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
