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KURVS: the outer rotation curve shapes and dark matter fractions of z ∼1.5 star-forming galaxies

Puglisi, A. (author)
Durham University,University of Southampton
Dudzeviciute, U. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Swinbank, Mark (author)
Durham University
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Gillman, S. (author)
Danmarks Tekniske Universitet,Technical University of Denmark
Tiley, Alfred L. (author)
Durham University,University of Western Australia
Bower, Richard G. (author)
Durham University
Cirasuolo, Michele (author)
European Southern Observatory (ESO)
Cortese, Luca (author)
University of Western Australia
Glazebrook, Karl (author)
Swinburne University of Technology
Harrison, C. M. (author)
University of Newcastle upon Tyne
Ibar, E. (author)
Universidad de Valparaíso,University of Valparaíso
Molina Tobar, Juan Andrés, 1991 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Obreschkow, Danail (author)
University of Western Australia
Oman, Kyle A. (author)
Durham University
Schaller, Matthieu (author)
Universiteit Leiden (UL),Leiden University (UL)
Shankar, F. (author)
University of Southampton
Sharples, R. (author)
Durham University
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 (creator_code:org_t)
2023
2023
English.
In: Monthly Notices of the Royal Astronomical Society. - 0035-8711 .- 1365-2966. ; 524:2, s. 2814-2835
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We present first results from the KMOS Ultra-deep Rotation Velocity Survey (KURVS), aimed at studying the outer rotation curves shape and dark matter content of 22 star-forming galaxies at z ∼1.5. These galaxies represent 'typical' star-forming discs at z ∼1.5, being located within the star-forming main sequence and stellar mass-size relation with stellar masses 9.5 ≤ log(M*/M⊙) ≤ 11.5. We use the spatially resolved H α emission to extract individual rotation curves out to 4 times the effective radius, on average, or ∼10-15 kpc. Most rotation curves are flat or rising between three and six disc scale radii. Only three objects with dispersion-dominated dynamics (vrot/σ0 ∼0.2) have declining outer rotation curves at more than 5σ significance. After accounting for seeing and pressure support, the nine rotation-dominated discs with vrot/σ0 ≥ 1.5 have average dark matter fractions of at the effective radius, similar to local discs. Together with previous observations of star-forming galaxies at cosmic noon, our measurements suggest a trend of declining dark matter fraction with increasing stellar mass and stellar mass surface density at the effective radius. Measurements of simulated EAGLE galaxies are in quantitative agreement with observations up to log, and overpredict the dark matter fraction of galaxies with higher mass surface densities by a factor of ∼3. We conclude that the dynamics of typical rotationally-supported discs at z ∼1.5 is dominated by dark matter from effective radius scales, in broad agreement with cosmological models. The tension with observations at high stellar mass surface density suggests that the prescriptions for baryonic processes occurring in the most massive galaxies (such as bulge growth and quenching) need to be reassessed.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

galaxies: high-redshift
galaxies: kinematics and dynamics
galaxies: evolution

Publication and Content Type

art (subject category)
ref (subject category)

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