Extremely High Excitation SiO Lines in Disk-outflow Systems in Orion Source I
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/872/i=1/a=64/pdf
Reference36 articles.
1. EXPLOSIVE OUTFLOWS POWERED BY THE DECAY OF NON-HIERARCHICAL MULTIPLE SYSTEMS OF MASSIVE STARS: ORION BN/KL
2. High-excitation SiO maser emission in VY Canis Majoris - Detection of the V = 4 J = 5-4 transition
3. GRAVITATIONAL SLINGSHOT OF YOUNG MASSIVE STARS IN ORION
4. ALMA spectral line and imaging survey of a low and a high mass-loss rate AGB star between 335 and 362 GHz
5. A Keplerian Disk around Orion SrCI, a ∼ 15 M ⊙ YSO
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1. Structure of the Source I Disk in Orion-KL;The Astrophysical Journal;2022-01-01
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. OMC-1 dust polarization in ALMA Band 7: diagnosing grain alignment mechanisms in the vicinity of Orion Source I;Monthly Notices of the Royal Astronomical Society;2021-03-04
4. Magnetic Field Structure of Orion Source I;The Astrophysical Journal;2020-06-24
5. Formation and Evolution of Disks Around Young Stellar Objects;Space Science Reviews;2020-04
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