Correlation between SiO v = 3 J = 1 → 0 maser excitation and the light curve of a long-period variable star-Reference-Cited by-同舟云学术

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Correlation between SiO v = 3 J = 1 → 0 maser excitation and the light curve of a long-period variable star

Published:2018-03-22 Issue:3 Volume:70 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Oyadomari Miyako¹,Imai Hiroshi¹,Nagayama Takumi²,Oyama Tomoaki²,Matsumoto Naoko²,Nakashima Jun-ichi³,Cho Se-Hyung⁴

Affiliation:

1. Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Kagoshima 890-0065, Japan

2. Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-12 Hoshigaoka, Mizusawa, Oshu, Iwate 023-0861, Japan

3. Department of Astronomy and Geodesy, Ural Federal University, Lenin Ave. 51, Ekaterinburg 620000, Russia

4. Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 305-348, Korea

Funder

Ministry of Education

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/70/3/33/25054955/psy021.pdf

Reference23 articles.

1. NEAR-INFRARED OBSERVATIONS OF SiO MASER-EMITTING ASYMPTOTIC GIANT BRANCH (AGB) STARS

2. SiO Maser Survey of Late-Type Stars. II. Statistical Study

3. First Detection of the SiO (v= 3,J= 2–1) Maser Emission from χ Cygni

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Observational characteristics of SiO masers around VX Sgr;Research in Astronomy and Astrophysics;2020-12-01

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