The pumping mechanism for SiO masers

Physics

Scientific paper

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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.

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