G305.8 - 0.2 water vapor source - A young object

Details G305.8 - 0.2 water vapor source - A young object G305.8 - 0.2 water vapor source - A young object

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....102.1734v&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 102, Nov. 1991, p. 1734-1737. Research supported by FINEP and FAPESP.

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 H2O 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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