CO Excitation in High-z Main-sequence Analogues: Resolved CO(4−3)/CO(3−2) Line Ratios in DYNAMO Galaxies

The spectral line energy distribution of carbon monoxide contains information about the physical conditions of the star-forming molecular hydrogen gas; however, the relation to local radiation field properties is poorly constrained. Using ∼1–2 kpc scale Atacama Large Millimeter Array observations of...

Täydet tiedot

Bibliografiset tiedot

Päätekijät:	Laura Lenkić, Alberto D. Bolatto, Deanne B. Fisher, Roberto Abraham, Karl Glazebrook, Rodrigo Herrera-Camus, Rebecca C. Levy, Danail Obreschkow, Carolyn G. Volpert
Aineistotyyppi:	Artigo
Kieli:	Inglês
Julkaistu:	IOP Publishing 2023-01-01
Sarja:	The Astrophysical Journal
Aiheet:	Interstellar emissions Extragalactic astronomy Disk galaxies
Linkit:	https://doi.org/10.3847/1538-4357/acb3b2
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