Time variations of water vapor masers in star-forming regions

Details Time variations of water vapor masers in star-forming regions Time variations of water vapor masers in star-forming regions

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..393..197m&link_type=abstract

The seventh astrophysical conference: Star formation, near and far. AIP Conference Proceedings, Volume 393, pp. 197-200 (1997).

Astronomy and Astrophysics

Astrophysics

Circumstellar Shells, Clouds, And Expanding Envelopes, Circumstellar Masers, Interstellar Masers

Scientific paper

The results of observations of water vapor maser at 22.2 GHz made during of about 15 years are presented. The results show that anticorrelation between the fluxes of different spectral ranges as well as of different spectral features is a common phenomenon in Star-Forming Regions (SFR) masers. We interpret these results as indicating that partial saturation commonly occurs in SFR water vapor masers.

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