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

M. Oyadomari, H. Imai, T. Nagayama, T. Oyama, N. Matsumoto, Y. Tamura, J. Nakashima, S.-H. Cho

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.

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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  -