Survey of OH masers at 1665 and 1667 MHz. I - Galactic longitudes 326 deg to 340 deg

Details Survey of OH masers at 1665 and 1667 MHz. I - Galactic longitudes 326 deg to 340 deg Survey of OH masers at 1665 and 1667 MHz. I - Galactic longitudes 326 deg to 340 deg

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980aujph..33..639c&link_type=abstract

Australian Journal of Physics, vol. 33, Sept. 1980, p. 639-669.

Astronomy and Astrophysics

Astronomy

70

Absorption Spectra, Galactic Radio Waves, Hydroxyl Emission, Interstellar Masers, Polarized Electromagnetic Radiation, Circular Polarization, Hydrogen Clouds, Luminosity, Radiant Flux Density, Radio Sources (Astronomy), Supernova Remnants, Water Masers, Zeeman Effect

Scientific paper

Forty main-line OH emission sources were found between the 326 and 340 deg galactic plane longitudes. The line profiles of all sources are depicted; the variability and intensity ratio statistics of the ground state transitions are presented. The velocity structures were very varied, with the maximum range of 25 km/s; combined velocity and polarization results are compatible with a Zeeman splitting origin for circular polarization, yielding an estimate for the line-of-sight field strength of a few mG.

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