Accurate positions of OH emission sources

Details Accurate positions of OH emission sources Accurate positions of OH emission sources

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...206..440e&link_type=abstract

Astrophysical Journal, vol. 206, June 1, 1976, pt. 1, p. 440-442.

Astronomy and Astrophysics

Astronomy

26

Hydroxyl Emission, Interferometry, Interstellar Masers, Position (Location), Radio Sources (Astronomy), Position Errors

Scientific paper

The Owens Valley interferometer has been used to measure accurate positions for nine OH emission sources at 1612 MHz and four sources at 1665 MHz. The baseline was 244 m north-south. In addition to the very strong 1612-MHz emitter OH 26.5+0.6, eight sources from the survey of Winnberg et al. (1975) were measured. A position was measured for the 1665-MHz maser emission from IC 2162 (S255), and the position of the maser in W75N was remeasured.

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