Abstract
The Owens Valley interferometer has been used to measure accurate positions for 9 OH emission sources at 1612 MHz and 4 sources at 1665 MHz. The baseline was 244 meters north--south. In addition to the very strong 1612 emitter, OH26.5+0.6, 8 sources from the survey of Winnberg et al. (1973) were measured. These positions have been used in a search for infrared objects (results presented elsewhere). In addition, a position was measured for the 1665 maser emission from IC2162 (S255), and the position of the maser in W75N was remeasured. (GRA)
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 callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
