A Systematic Observational Study on Galactic Interstellar Ratio 18O/17O. I. C18O and C17O J = 1

A Systematic Observational Study on Galactic Interstellar Ratio 18O/17O. I. C18O and C17O J = 1–0 Data Analysis

Published:2020-06-26 Issue:1 Volume:249 Page:6
ISSN:1538-4365
Container-title:The Astrophysical Journal Supplement Series
language:
Short-container-title:ApJS

Author:

Zhang J. S.^ORCID,Liu W.,Yan Y. T.,Yu H. Z.,Liu J. T.,Zheng Y. H.,Romano D.^ORCID,Zhang Z.-Y.^ORCID,Wang J. Z.,Chen J. L.,Wang Y. X.,Zhang W. J.,Lu H. H.,Chen L. S.,Zou Y. P.,Yang H. Q.,Wen T.,Lu F. S.

Funder

Natural Science Foundation of China

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4365/ab9112/pdf

Reference36 articles.

1. Searching for Inflow toward Massive Starless Clump Candidates Identified in the Bolocam Galactic Plane Survey

2. Super and massive AGB stars – II. Nucleosynthesis and yields – Z = 0.02, 0.008 and 0.004

3. Super and massive AGB stars – III. Nucleosynthesis in metal-poor and very metal-poor stars – Z = 0.001 and 0.0001

4. Revisiting the radial abundance gradients of nitrogen and oxygen of the Milky Way

5. A measurement of the hyperfine structure of C17O

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