Physical Conditions in the LMC’s Quiescent Molecular Ridge: Fitting Non-LTE Models to CO Emission-Reference-Cited by-同舟云学术

Physical Conditions in the LMC’s Quiescent Molecular Ridge: Fitting Non-LTE Models to CO Emission

Published:2021-08-01 Issue:2 Volume:917 Page:106
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Finn Molly K.^ORCID,Indebetouw Remy^ORCID,Johnson Kelsey E.^ORCID,Costa Allison H.^ORCID,Chen C.-H. Rosie^ORCID,Kawamura Akiko^ORCID,Onishi Toshikazu^ORCID,Ott Jürgen^ORCID,Tokuda Kazuki^ORCID,Wong Tony^ORCID,Zahorecz Sarolta^ORCID

Funder

National Science Foundation

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ac090c/pdf

Reference67 articles.

1. Astropy: A community Python package for astronomy

2. Integrated UBV Photometry of 624 Star Clusters and Associations in the Large Magellanic Cloud

3. The CO-to-H2 Conversion Factor

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