G305.8 - 0.2 water vapour source: A young object

Details G305.8 - 0.2 water vapour source: A young object G305.8 - 0.2 water vapour source: A young object

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991stin...9231343v&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Protostars, Stellar Evolution, Water Masers, Early Stars, Infrared Astronomy Satellite, Silicon Oxides, Southern Sky

Scientific paper

Observations of water vapor and silicon monoxide masers were conducted in the direction of G305.8-0.2. No SiO maser emission above 7 Jy of flux density was detected. The short-time variability of the H20 maser together with the absence of compact radio continuum emission suggests that the excitation energy of the maser could originate from an O7-O9 protostar in its earlier evolutionary stages.

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