Turbulent Motions of H_2O Masers

Details Turbulent Motions of H_2O Masers Turbulent Motions of H_2O Masers

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...182.3707g&link_type=abstract

American Astronomical Society, 182nd AAS Meeting, #37.07; Bulletin of the American Astronomical Society, Vol. 25, p.855

Astronomy and Astrophysics

Astronomy

Scientific paper

H_2O masers appear where strong winds from young massive stars strike ambient material. Observations of positions, proper motions and Doppler shifts of maser features trace motions of the interacting material. Correlation functions of these observables show the scale-free structure characteristic of self-similar turbulence, down to a minimum scale of about an AU. We compare observational results with theoretical models for supersonic turbulence.

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