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STATISTICAL STUDIES BASED ON SIMULTANEOUS SiO AND H2O MASER SURVEYS TOWARD EVOLVED STARS

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Variations of the [FORMULA][F]v[/F][/FORMULA] = 0, 1, 2, and 3, J  = 1-0 SiO Masers of Mira

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Axial Symmetry and Rotation in the SiO Maser Shell of IK Tauri

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Time Variation of SiO Masers in VX Sagittarii over an Optically Quiescent Phase

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First mm-VLBI Observations between the TRAO 14-m and the NRO 45-m Telescopes: Observations of 86 GHz SiO Masers in VY Canis Majoris

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Continuous and burst-like accretion on to substellar companions in Mira winds

Curtis Struck, Babak E. Cohanim and Lee Anne Willson
Monthly Notices of the Royal Astronomical Society 347 (1) 173 (2004)
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Using VLBI to Probe the Orion KL Outflow on AU Scales

Sheperd S. Doeleman, Colin J. Lonsdale, Paul T. Kondratko and C. Read Predmore
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High resolution observations of SiO masers: Comparing the spatial distribution at 43 and 86 GHz

R. Soria-Ruiz, J. Alcolea, F. Colomer, et al.
Astronomy & Astrophysics 426 (1) 131 (2004)
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$\boldmath\mathsf{^{28}}$SiOv = 1 andv = 2,J = 1–0 maser variability in evolved stars. Eleven years of short spaced monitoring

J. R. Pardo, J. Alcolea, V. Bujarrabal, et al.
Astronomy & Astrophysics 424 (1) 145 (2004)
https://doi.org/10.1051/0004-6361:20040309

Mass-Losing Pulsating Stars and their Circumstellar Matter

E. M. L. Humphreys, M.D Gray, J.A Yates, et al.
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https://doi.org/10.1007/978-94-010-0139-7_69

R Cassiopeiae: Relative Strengths of SiO Masers at 43 and 86 GHz

R. B. Phillips, A. H. Straughn, S. S. Doeleman and C. J. Lonsdale
The Astrophysical Journal 588 (2) L105 (2003)
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Mass-Losing Pulsating Stars and their Circumstellar Matter

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A Polarization Survey of SiO Maser Variability in Evolved Stars

J. Glenn, P. R. Jewell, R. Fourre and L. Miaja
The Astrophysical Journal 588 (1) 478 (2003)
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Mass-Losing Pulsating Stars and their Circumstellar Matter

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https://doi.org/10.1007/978-94-010-0139-7_65

A Movie of a Star: Multiepoch Very Long Baseline Array Imaging of the SiO Masers toward the Mira Variable TX Cam

P. J. Diamond and A. J. Kemball
The Astrophysical Journal 599 (2) 1372 (2003)
https://doi.org/10.1086/379347