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## Correlation of the Relative SiO Maser Distributions with the Stellar Light Curves

Труды ИПА РАН, вып. 41, 95–98 (2017)

Ключевые слова: AGB stars, SiO masers

### Аннотация

We carried out VLBI observations of SiO v = 2 and v = 3 J = 1 → 0 masers towards 12 long-period variables (LPVs) using four telescopes of the VLBI Exploration of Radio Astrometry (VERA) combined with the Nobeyama 45 m telescope. We found some correlation of the relative maser distributions with the stellar light curves. The location of the v = 2 masers coincide with the v = 3 masers region at pulsation phase ϕ = 0.0 − 0.2.

### Цитирование

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M. Oyadomari, H. Imai, T. Nagayama, T. Oyama, N. Matsumoto, Y. Tamura, J. Nakashima, S.-H. Cho. Correlation of the Relative SiO Maser Distributions with the Stellar Light Curves // Труды ИПА РАН. — 2017. — Вып. 41. — С. 95–98. @article{oyadomari2017, abstract = {We carried out VLBI observations of SiO v = 2 and v = 3 J = 1 → 0 masers towards 12 long-period variables (LPVs) using four telescopes of the VLBI Exploration of Radio Astrometry (VERA) combined with the Nobeyama 45 m telescope. We found some correlation of the relative maser distributions with the stellar light curves. The location of the v = 2 masers coincide with the v = 3 masers region at pulsation phase ϕ = 0.0 − 0.2.}, author = {M. Oyadomari and H. Imai and T. Nagayama and T. Oyama and N. Matsumoto and Y. Tamura and J. Nakashima and S.~-H. Cho}, issue = {41}, journal = {Труды ИПА РАН}, keyword = {AGB stars, SiO masers}, pages = {95--98}, title = {Correlation of the Relative SiO Maser Distributions with the Stellar Light Curves}, url = {http://iaaras.ru/library/paper/1712/}, year = {2017} } TY - JOUR TI - Correlation of the Relative SiO Maser Distributions with the Stellar Light Curves AU - Oyadomari, M. AU - Imai, H. AU - Nagayama, T. AU - Oyama, T. AU - Matsumoto, N. AU - Tamura, Y. AU - Nakashima, J. AU - Cho, S. -H. PY - 2017 T2 - Труды ИПА РАН IS - 41 SP - 95 AB - We carried out VLBI observations of SiO v = 2 and v = 3 J = 1 → 0 masers towards 12 long-period variables (LPVs) using four telescopes of the VLBI Exploration of Radio Astrometry (VERA) combined with the Nobeyama 45 m telescope. We found some correlation of the relative maser distributions with the stellar light curves. The location of the v = 2 masers coincide with the v = 3 masers region at pulsation phase ϕ = 0.0 − 0.2. UR - http://iaaras.ru/library/paper/1712/ ER -