Monitoring of water masers from IRAS sources

Details Monitoring of water masers from IRAS sources Monitoring of water masers from IRAS sources

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990iau..conf.....s&link_type=abstract

Presented at the VI Regional Latin-American of the IAU

Astronomy and Astrophysics

Astronomy

Dust, Pre-Main Sequence Stars, Southern Hemisphere, Star Formation, Water Masers, Water Vapor, Infrared Astronomy Satellite, Spectrum Analysis, Surveys

Scientific paper

Twenty-three water vapor masers in the direction of IRAS sources in the Southern Hemisphere had their intensities monitored systematically at Itapetinga Radio Observatory. These masers were detected in four surveys in which each run had different selection criteria. The IRAS fluxes analysis and the shape of the spectra of these masers suggest that the objects are associated with premain sequence stars, still surrounded by the dust cocoon. Almost all sources presented drastic changes in the overall spectral line distribution in their spectra.

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