Physics
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atnf.prop.1749d&link_type=abstract
ATNF proposal C1953, Semester: October, 2008
Physics
Stellar, Galactic, Atca
Scientific paper
We will observe a selected list of SiO masers at 3 and 7mm co-temporally. We will monitor the evolution of the fluxes in the different frequencies and find the relationship between them. There are two completing models for SiO maser pumping, each requiring very different physical conditions in the inner circumstellar layers to reproduce the observed emission. With this monitoring experiment we aim to determine which model is correct because we will be able to deduce the travel time of the pumping mechanism.
Bujarrabal Valentin
Dodson Richard
Rioja Maria
Voronko Maxim
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