Mapping the Outflow from G5.89-0.39 in SiO J = 5 → 4-Reference-Cited by-同舟云学术

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Mapping the Outflow from G5.89-0.39 in SiO J = 5 → 4

Published:2004-10-28 Issue:1 Volume:616 Page:L35-L38
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Sollins P. K.,Hunter T. R.,Battat J.,Beuther H.,Ho P. T. P.,Lim J.,Liu S. Y.,Ohashi N.,Sridharan T. K.,Su Y. N.,Zhao J.-H.,Zhang Q.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference32 articles.

1. The Expansion Rate of and Distance to G5.89−0.39

2. The Extraordinary Outflow toward G5.89−0.39

3. Lifetimes of Ultracompact H II Regions: High-Resolution Methyl Cyanide Observations

4. The Mass-Velocity and Position-Velocity Relations in Episodic Outflows

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1. SiO outflows in the most luminous and massive protostellar sources of the southern sky;Astronomy & Astrophysics;2023-09

2. Imaging Molecular Outflow in Massive Star-forming Regions with HNCO Lines;The Astrophysical Journal;2023-06-01

3. Magnetic Fields in Massive Star-forming Regions (MagMaR). I. Linear Polarized Imaging of the Ultracompact H ii Region G5.89–0.39;The Astrophysical Journal;2021-05-01

4. Confirming the Explosive Outflow in G5.89 with ALMA;The Astrophysical Journal;2020-10-22

5. Protostellar Outflows at the EarliesT Stages (POETS);Astronomy & Astrophysics;2019-10-22

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