An oh Gigamaser in the Source PHL:909

Details An oh Gigamaser in the Source PHL:909 An oh Gigamaser in the Source PHL:909

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sva....36..669v&link_type=abstract

Soviet Astronomy, Vol.36, NO. 6/NOV, P.669, 1992

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the results of a search for OH emission in the quasistellar galaxy PHL 909 with the RATAN-600 radio telescope. A signal with an antenna temperature (25 +/- 5) mK and a profile width of about 900 kHz, which corresponds to a flux density (60 +/- 12) microJy, has probably been observed in two observing runs. For H_0_ = 75 km/(sec x Mpc), the source's isotropic luminosity in this line is 0.8 x 10^4^ L_sun_.

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