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Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago

Authors :
N. M. Förster Schreiber
Philipp Lang
Sandro Tacchella
Emily Wisnioski
Hannah Übler
Tal Alexander
Shy Genel
Alessandra Beifiori
C. M. Carollo
Sirio Belli
Ortwin Gerhard
Reinhard Genzel
Linda J. Tacconi
Andreas Burkert
Gabriel B. Brammer
Amiel Sternberg
Ralf Bender
Dieter Lutz
T. Naab
J. T. Mendel
Jeffrey C. C. Chan
Alvio Renzini
David J. Wilman
Matteo Fossati
Richard Davies
Ken-ichi Tadaki
Audrey Galametz
Stijn Wuyts
Ivelina Momcheva
Erica J. Nelson
Roberto P. Saglia
Genzel, R
Schreiber, N
Ubler, H
Lang, P
Naab, T
Bender, R
Tacconi, L
Wisnioski, E
Wuyts, S
Alexander, T
Beifiori, A
Belli, S
Brammer, G
Burkert, A
Carollo, C
Chan, J
Davies, R
Fossati, M
Galametz, A
Genel, S
Gerhard, O
Lutz, D
Mendel, J
Momcheva, I
Nelson, E
Renzini, A
Saglia, R
Sternberg, A
Tacchella, S
Tadaki, K
Wilman, D
Source :
Genzel, R, Schreiber, N M F, Übler, H, Lang, P, Naab, T, Bender, R, Tacconi, L J, Wisnioski, E, Wuyts, S, Alexander, T, Beifiori, A, Belli, S, Brammer, G, Burkert, A, Carollo, C M, Chan, J, Davies, R, Fossati, M, Galametz, A, Genel, S, Gerhard, O, Lutz, D, Mendel, J T, Momcheva, I, Nelson, E J, Renzini, A, Saglia, R, Sternberg, A, Tacchella, S, Tadaki, K & Wilman, D 2017, ' Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago ', Nature, vol. 543, no. 7645, pp. 397-401 . https://doi.org/10.1038/nature21685
Publication Year :
2016

Abstract

In cold dark matter cosmology, the baryonic components of galaxies are thought to be mixed with and embedded in non-baryonic and non-relativistic dark matter, which dominates the total mass of the galaxy and its dark matter halo. In the local Universe, the mass of dark matter within a galactic disk increases with disk radius, becoming appreciable and then dominant in the outer, baryonic regions of the disks of star-forming galaxies. This results in rotation velocities of the visible matter within the disk that are constant or increasing with disk radius. Comparison between the dynamical mass and the sum of stellar and cold gas mass at the peak epoch of galaxy formation, inferred from ancillary data, suggest high baryon factions in the inner, star-forming regions of the disks. Although this implied baryon fraction may be larger than in the local Universe, the systematic uncertainties (stellar initial mass function, calibration of gas masses) render such comparisons inconclusive in terms of the mass of dark matter. Here we report rotation curves for the outer disks of six massive star-forming galaxies, and find that the rotation velocities are not constant, but decrease with radius. We propose that this trend arises because of two main factors: first, a large fraction of the massive, high-redshift galaxy population was strongly baryon dominated, with dark matter playing a smaller part than in the local Universe; and second, the large velocity dispersion in high-redshift disks introduces a substantial pressure term that leads to a decrease in rotation velocity with increasing radius. The effect of both factors appears to increase with redshift. Qualitatively, the observations suggest that baryons in the early Universe efficiently condensed at the centres of dark matter halos when gas fractions were high, and dark matter was less concentrated. [Abridged]<br />Accepted for publication in Nature. Note press embargo until 1800 London time / 1400 US Eastern Time on 15 March 2017

Details

ISSN :
14764687
Volume :
543
Issue :
7645
Database :
OpenAIRE
Journal :
Nature
Accession number :
edsair.doi.dedup.....48cca94cabd4613f30a00457d0bc10e7
Full Text :
https://doi.org/10.1038/nature21685