High-excitation SiO maser emission in VY Canis Majoris - Detection of the V = 4 J = 5-4 transition
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 41 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. Vibrationally excited HCN transitions in circumstellar envelopes of carbon-rich AGB stars;Astronomy & Astrophysics;2022-10
2. SiO, 29SiO, and 30SiO Emission from 67 Oxygen-rich Stars: A Survey of 61 Maser Lines from 7 to 1 mm;The Astrophysical Journal Supplement Series;2021-03-26
3. Extremely High Excitation SiO Lines in Disk-outflow Systems in Orion Source I;The Astrophysical Journal;2019-02-11
4. The Maser-emitting Structure and Time Variability of the SiS Lines J = 14–13 and 15–14 in IRC+10216;The Astrophysical Journal;2018-06-25
5. Strong magnetic field generated by the extreme oxygen-rich red supergiant VY Canis Majoris;Publications of the Astronomical Society of Japan;2017-11-17
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