The Structure and Polarization Properties of the SiO Masers in the Extended Atmosphere of R Aquarii
Silicon monoxide (SiO) maser emission has been observed towards many late-type stars. The conditions necessary for the formation of SiO masers dictate that they be produced in a region which is inside the silicate dust formation point close to the surface of the star. Very Long Baseline Interferom...
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| Format: | Others |
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Virginia Tech
2014
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| Online Access: | http://hdl.handle.net/10919/30630 http://scholar.lib.vt.edu/theses/available/etd-61797-104237/ |