CH3OH and H2O masers in high-mass star-forming regions
arXiv:astro-ph/0205348 · doi:10.1051/0004-6361:20020710
Abstract
We present a comparison of ClassII CH3OH and H2O masers at high spatial resolution in a sample of 29 massive star-forming regions. Absolute positions of both maser types are compared with mm dust continuum, cm continuum and mid-infrared sources. Spatial correlations of the different tracers and kinematic signatures are discussed.
12 pages, 5 figures, accepted by Astronomy and Astrophysics