| http://www.w3.org/ns/prov#value | - If we can find H2O masers at different wavelengths in the same volumes of gas as those emitting at centimeter wavelengths, then we can define conditions there such as gas temperature and density much better, said Mark J. Reid of CfA. If we find them in different volumes as well, then we can trace uncharted regions of the active galactic nucleus, including those closer to the central black hole.
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