Kiloparsec view of a typical star-forming galaxy when the Universe was similar 
to 1 Gyr old - II. Regular rotating disk and evidence for baryon dominance on 
galactic scales

Herrera-Camus, R.; Schreiber, N. M. Förster; Price, S. H.; Übler, H.; Bolatto, A. D.; Davies, R. L.; Fisher, D.; Genzel, R.; Lutz, D.; Naab, T.; Nestor, A.; Shimizu, T.; Sternberg, A.; Tacconi, L.; Tadaki, K.

doi:10.1051/0004-6361/202142562

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Kiloparsec view of a typical star-forming galaxy when the Universe was similar to 1 Gyr old - II. Regular rotating disk and evidence for baryon dominance on galactic scales

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Naab, T.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Herrera-Camus, R., Schreiber, N. M. F., Price, S. H., Übler, H., Bolatto, A. D., Davies, R. L., et al. (2022). Kiloparsec view of a typical star-forming galaxy when the Universe was similar to 1 Gyr old - II. Regular rotating disk and evidence for baryon dominance on galactic scales. Astronomy and Astrophysics, 665: L8. doi:10.1051/0004-6361/202142562.

Cite as: https://hdl.handle.net/21.11116/0000-000B-5CC0-5

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