EVIDENCE FOR STABLE v=0, J=1 → 0 SiO MASER EMISSION FROM VY CANIS MAJORIS

Observations of the SiO v = 0, J = 1 -> 0 spectra from VY CMa from 2003 through 2006 indicate an unusually long-lived, highly linearly polarized maser emission at a V-lsr of approximately 18.5 km s(-1). A time series cross-correlation analysis has been developed for calculating the characteristic lifetime of linearly polarized spectra. Applying the cross-correlation to these spectra indicates a characteristic lifetime of 5600 +/- 400 days. These emission characteristics may be generated in a region of relatively stable outflow geometry and magnetic field rather than in the more ephemeral circumstellar environment.