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The chemical structure of young high-mass star-forming cl... | ResearchHub
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The chemical structure of young high-mass star-forming clumps: (II) parsec-scale CO depletion and deuterium fraction of $\rm HCO^+$
0
Authors
Siyi Feng
21 more
Siyi Feng
•
Dong Li
19 more
•
Jinghua Yuan
Published
September 28, 2020
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Preprint Server
Topics
Astrophysics
Atomic Physics
Physics
Chemistry
Astrochemistry
Show all topics
DOI
10.3847/1538-4357/abada3
License
arXiv License
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Support the authors with ResearchCoin
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Preprint Server
Topics
Astrophysics
Atomic Physics
Physics
Chemistry
Astrochemistry
Show all topics
DOI
10.3847/1538-4357/abada3
License
arXiv License
