A search for SiO masers in Orion-like regions

Details A search for SiO masers in Orion-like regions A search for SiO masers in Orion-like regions

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aj.....89.1833b&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 89, Dec. 1984, p. 1833-1835.

Astronomy and Astrophysics

Astronomy

19

Interstellar Masers, Orion Nebula, Radio Astronomy, Silicon Oxides, Late Stars, Luminosity, Radiant Flux Density, Stellar Evolution

Scientific paper

A sensitive search for SiO maser emission toward objects possessing high-velocity flows and/or disk geometries has revealed no Orion-like sources. The ratios of the luminosity limits reported here to the Orion SiO maser luminosity range from 0.04 to 0.0002, indicating that the Orion masers are associated with a unique set of physical conditions and not any widespread phenomena, even at a weak level. The authors report detection of a new SiO maser toward the reflection nebula OH231.8+4.2, exhibiting characteristics typical of the SiO masers seen toward late-type stars.

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