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Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago
- 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
- Subjects :
- Cold dark matter
Dark matter
Scalar field dark matter
galaxy evolution
FOS: Physical sciences
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
0103 physical sciences
Galaxy formation and evolution
General
010303 astronomy & astrophysics
Galaxy rotation curve
Astrophysics::Galaxy Astrophysics
Physics
Medicine(all)
Multidisciplinary
010308 nuclear & particles physics
Hot dark matter
Astronomy
Astrophysics - Astrophysics of Galaxies
Dark matter halo
kinematics
Astrophysics of Galaxies (astro-ph.GA)
Dark galaxy
Astrophysics::Earth and Planetary Astrophysics
Subjects
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