Exploring the CO/CN line ratio in nearby galaxies with the ALMA archive
Author:
Affiliation:
1. Department of Physics and Astronomy, McMaster University, 1280 Main St. W., Hamilton, Ontario L8S 4M1, Canada
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/477/3/2926/24803119/sty845.pdf
Reference59 articles.
Cited by 14 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Molecular Gas and the Star-Formation Process on Cloud Scales in Nearby Galaxies;Annual Review of Astronomy and Astrophysics;2024-09-13
2. Absorption of Millimeter-band CO and CN in the Early Universe: Molecular Clouds in the Radio Galaxy B2 0902+34 at Redshift 3.4;The Astrophysical Journal;2024-02-01
3. Stored in the archives: Uncovering the CN/CO intensity ratio with ALMA in nearby U/LIRGs;Monthly Notices of the Royal Astronomical Society;2023-11-03
4. A nearly constant CN/HCN line ratio in nearby galaxies: CN as a new tracer of dense gas;Monthly Notices of the Royal Astronomical Society;2023-02-22
5. Young Radio Sources Expanding in Gas-Rich ISM: Using Cold Molecular Gas to Trace Their Impact;Galaxies;2023-02-02
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