Molecular clouds in the Cosmic Snake normal star-forming galaxy 8 billion years ago

@article{DessaugesZavadsky2019MolecularCI,
  title={Molecular clouds in the Cosmic Snake normal star-forming galaxy 8 billion years ago},
  author={Miroslava Dessauges-Zavadsky and Johan Richard and Françoise Combes and Daniel Schaerer and Wiphu Rujopakarn and Lucio Mayer and Antonio Cava and Fr'ed'eric Boone and E. Egami and Jean-Paul Kneib and Pablo G. P'erez-Gonz'alez and Daniel HuberDaniel Pfenniger and Timothy D. Rawle and R. Teyssier and Paul P. van der Werf},
  journal={Nature Astronomy},
  year={2019}
}
The cold molecular gas in contemporary galaxies is structured in discrete cloud complexes. These giant molecular clouds (GMCs), with 104–107 solar masses (M⊙) and radii of 5–100 parsecs, are the seeds of star formation1. Highlighting the molecular gas structure at such small scales in distant galaxies is observationally challenging. Only a handful of molecular clouds were reported in two extreme submillimetre galaxies at high redshift2–4. Here we search for GMCs in a typical Milky Way… 

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