CH3OH and H2O masers in high-mass star-forming regions
Preprint
- 21 May 2002
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.Keywords
All Related Versions
- Version 1, 2002-05-21, ArXiv
- Published version: Astronomy & Astrophysics, 390 (1), 289.
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