Observations of the new OH maser source G43.2-0.1

Details Observations of the new OH maser source G43.2-0.1 Observations of the new OH maser source G43.2-0.1

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..362p&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, June 1982, p. 362-364.) Soviet Astronomy Letters, vol. 8, May-June 1982, p. 196, 197

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Emission Spectra, Hydrogen Clouds, Hydroxyl Emission, Interstellar Masers, Radio Sources (Astronomy), Centimeter Waves, Circular Polarization

Scientific paper

Emission in the 1612-MHz OH line has been recorded with the Nancay radio telescope in the new maser source G43.2-0.1, which is located in the same direction as the radio complex W49. The emission is weakly circularly polarized and peaks at two radial velocities, 35.8 and 62.6 km/sec. No emission has been detected in the other three 18-cm OH lines or in the 1.35-cm H2O line. The maser G43.2-0.1 has characteristics resembling type II OH/IR sources. It cannot be identified with any known variable or infrared star.

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