Detection of H2O emission from galaxy NGC253

Physics

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Galactic Radiation, Microwave Spectra, Radio Emission, Radio Galaxies, Water Vapor, Hydroxyl Emission, Radial Velocity, Radiant Flux Density

Scientific paper

This letter reports the detection of the 6(16) - 5(23) transition of water vapor at 22.235 GHz in NGC 253, a large edge-on spiral galaxy located at a distance of 3.4 Mpc. The observations were performed using a double-sideband balanced-mixer receiver with a system temperature of about 1000 K and a 46-channel filter bank having a resolution of 100 kHz. An H2O spectrum of NGC 253 is presented which exhibits an emission feature of 5.2 (plus or minus 1.2) Jy at a radial velocity of 233 km/s. It is suggested that this emission feature may be associated with 1667-MHz OH emission previously observed at 239 km/s. The intrinsic power of the H2O emission at 233 km/s is shown to be about three times greater than that of W49 during its maxima.

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