We present single-dish monitoring of the spectra of 13 extragalactic water megamasers taken over a period of 9 years and a single epoch of sensitive spectra for 7 others. Our data include the first K-band science observations taken with the new 100 m Green Bank Telescope (GBT). In the context of a circumnuclear, molecular disk model, our results suggest that either (a) the maser lines seen are systemic features subject to a much smaller acceleration than present in NGC 4258, presumably because the gas is farther from the nuclear black hole, or (b) we are detecting ``satellite'' lines for which the acceleration is in the plane of the sky. We also report a search for water vapor masers towards the nuclei of 58 highly inclined, nearby galaxies.
CITATION STYLE
Braatz, J. A., Wilson, A. S., Henkel, C., Gough, R., & Sinclair, M. (2003). A Survey for H 2 O Megamasers. III. Monitoring Water Vapor Masers in Active Galaxies. The Astrophysical Journal Supplement Series, 146(2), 249–265. https://doi.org/10.1086/374417
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