Author
Listed:
- R. Genzel
(Max-Planck-Institut für extraterrestrische Physik (MPE)
University of California)
- N. M. Förster Schreiber
(Max-Planck-Institut für extraterrestrische Physik (MPE))
- H. Übler
(Max-Planck-Institut für extraterrestrische Physik (MPE))
- P. Lang
(Max-Planck-Institut für extraterrestrische Physik (MPE))
- T. Naab
(Max-Planck Institute for Astrophysics)
- R. Bender
(Max-Planck-Institut für extraterrestrische Physik (MPE)
Universitäts-Sternwarte Ludwig-Maximilians-Universität (USM))
- L. J. Tacconi
(Max-Planck-Institut für extraterrestrische Physik (MPE))
- E. Wisnioski
(Max-Planck-Institut für extraterrestrische Physik (MPE))
- S. Wuyts
(Max-Planck-Institut für extraterrestrische Physik (MPE)
University of Bath)
- T. Alexander
(Faculty of Physics, The Weizmann Institute of Science)
- A. Beifiori
(Max-Planck-Institut für extraterrestrische Physik (MPE)
Universitäts-Sternwarte Ludwig-Maximilians-Universität (USM))
- S. Belli
(Max-Planck-Institut für extraterrestrische Physik (MPE))
- G. Brammer
(Space Telescope Science Institute)
- A. Burkert
(Max-Planck-Institut für extraterrestrische Physik (MPE)
Max-Planck Institute for Astrophysics)
- C. M. Carollo
(Institute of Astronomy, Eidgenössische Technische Hochschule, ETH Zürich)
- J. Chan
(Max-Planck-Institut für extraterrestrische Physik (MPE))
- R. Davies
(Max-Planck-Institut für extraterrestrische Physik (MPE))
- M. Fossati
(Max-Planck-Institut für extraterrestrische Physik (MPE)
Universitäts-Sternwarte Ludwig-Maximilians-Universität (USM))
- A. Galametz
(Max-Planck-Institut für extraterrestrische Physik (MPE)
Universitäts-Sternwarte Ludwig-Maximilians-Universität (USM))
- S. Genel
(Center for Computational Astrophysics)
- O. Gerhard
(Max-Planck-Institut für extraterrestrische Physik (MPE))
- D. Lutz
(Max-Planck-Institut für extraterrestrische Physik (MPE))
- J. T. Mendel
(Max-Planck-Institut für extraterrestrische Physik (MPE)
Universitäts-Sternwarte Ludwig-Maximilians-Universität (USM))
- I. Momcheva
(Yale University)
- E. J. Nelson
(Max-Planck-Institut für extraterrestrische Physik (MPE)
Yale University)
- A. Renzini
(Osservatorio Astronomico di Padova)
- R. Saglia
(Max-Planck-Institut für extraterrestrische Physik (MPE)
Universitäts-Sternwarte Ludwig-Maximilians-Universität (USM))
- A. Sternberg
(School of Physics and Astronomy, Tel Aviv University)
- S. Tacchella
(Institute of Astronomy, Eidgenössische Technische Hochschule, ETH Zürich)
- K. Tadaki
(Max-Planck-Institut für extraterrestrische Physik (MPE))
- D. Wilman
(Max-Planck-Institut für extraterrestrische Physik (MPE)
Universitäts-Sternwarte Ludwig-Maximilians-Universität (USM))
Abstract
The rotation velocities in the outer disks of six massive star-forming galaxies are shown to decrease with disk radius, owing to high baryonic mass fractions and large velocity dispersions.
Suggested Citation
R. Genzel & N. M. Förster Schreiber & H. Übler & P. Lang & T. Naab & R. Bender & L. J. Tacconi & E. Wisnioski & S. Wuyts & T. Alexander & A. Beifiori & S. Belli & G. Brammer & A. Burkert & C. M. Carol, 2017.
"Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago,"
Nature, Nature, vol. 543(7645), pages 397-401, March.
Handle:
RePEc:nat:nature:v:543:y:2017:i:7645:d:10.1038_nature21685
DOI: 10.1038/nature21685
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