Galactic Water Vapor Emission: Further Observations of Variability
S. H. Knowles 1,
C. H. Mayer 1,
W. T. Sullivan III 1, and
A. C. Cheung 2
1 E. O. Hulburt Center for Space Research, Naval Research Laboratory, Washington, D.C. 20390
2 Department of Physics, University of California. Berkeley 94720
Recent observations of the 1.35-centimeter line emission of water vapor from galactic sources show short-term variability in the spectra of several sources. Two additional sources, Cygnus 1 and NGC 6334N, have been observed, and the spectra of W49 and VY Canis Majoris were measured over a wider range of radial velocity.