The properties of the interstellar medium in dusty, star-forming galaxies at $z \sim 2-4$: The shape of the CO spectral line energy distributions

Fuente: arXiv

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Bibliographic Details
Main Authors:	Taylor, Dominic J., Swinbank, A. M., Smail, Ian, Puglisi, Annagrazia, Birkin, Jack E., Dudzeviciute, Ugne, Chen, Chian-Chou, Ikarashi, S., Castillo, Marta Frias, Weiss, Axel, Li, Zefeng, Chapman, Scott C., Jansen, Jasper, Jimenez-Andrade, E. F., Morabito, Leah K., Murphy, Eric J., Rybak, Matus, van der Werf, P. P.
Format:	Preprint
Published:	2024
Subjects:	Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2411.14271