The OH gigamaser in the source PHL 909

Details The OH gigamaser in the source PHL 909 The OH gigamaser in the source PHL 909

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992azh....69.1313v&link_type=abstract

Astronomicheskij Zhurnal (ISSN 0004-6299), vol. 69, no. 6, p. 1313, 1314.

Astronomy and Astrophysics

Astronomy

Hydroxyl Emission, Interstellar Masers, Radio Telescopes, Autocorrelation, Radio Spectra

Scientific paper

Results of a search with the RATAN-600 radiotelescope for powerful OH emission in the quasi-stellar galaxy PHL 909 are reported. A signal with an antenna temperature of (25 +/- 5 mK) and a spectral width of 900 kHz was probably found in two observational cycles. The flux density of this signal is (60 +/- 12) mJy. With H(0) = 75 km/s Mpc the isotropic luminosity of the source in this line is 0.8 x 10 exp 4 solar luminosities.

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