High-Velocity H2O Masers Associated Massive Star Formation Regions

Details High-Velocity H2O Masers Associated Massive Star Formation Regions High-Velocity H2O Masers Associated Massive Star Formation Regions

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001chphl..18.1663x&link_type=abstract

Chinese Physics Letters, Volume 18, Issue 12, pp. 1663-1665 (2001).

Physics

Scientific paper

We report on the results of 12CO (1-0) emission associated with H2O masers and massive star formation regions to identify high-velocity H2O masers. Several masers have a large blueshift, even up to 120 km.s-1, with respect to the CO peak, but no large redshifted maser appears. This result suggests that high-velocity H2O masers can most probably occur in high mass star-forming regions and quite a number of masers stem from the amplifications of a background source, which may enable those undetectable weak masers to come to an observable level.

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