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Emergence and cosmic evolution of the Kennicutt- Schmidt relation driven by interstellar turbulence

Kraljic, Katarina (author)
Observatory of Strasbourg
Renaud, Florent (author)
Lund University,Lunds universitet,Astrofysik,Fysiska institutionen,Institutioner vid LTH,Lunds Tekniska Högskola,Astrophysics,Department of Physics,Departments at LTH,Faculty of Engineering, LTH,University of Strasbourg,Observatory of Strasbourg
Dubois, Yohan (author)
Paris-Sorbonne University
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Pichon, Christophe (author)
Institut de Physique Théorique,Paris-Sorbonne University,Korea Institute for Advanced Study
Agertz, Oscar (author)
Lund University,Lunds universitet,Astrofysik,Fysiska institutionen,Institutioner vid LTH,Lunds Tekniska Högskola,Astrophysics,Department of Physics,Departments at LTH,Faculty of Engineering, LTH
Andersson, Eric (author)
American Museum of Natural History
Devriendt, Julien (author)
University of Oxford
Freundlich, Jonathan (author)
Observatory of Strasbourg
Kaviraj, Sugata (author)
University of Hertfordshire
Kimm, Taysun (author)
Yonsei University
Martin, Garreth (author)
University of Nottingham,Korea Astronomy and Space Science Institute (KASI),University of Arizona
Peirani, Sébastien (author)
Côte d'Azur Observatory
Segovia Otero, Álvaro (author)
Lund University,Lunds universitet,Astrofysik,Fysiska institutionen,Institutioner vid LTH,Lunds Tekniska Högskola,Astrophysics,Department of Physics,Departments at LTH,Faculty of Engineering, LTH
Volonteri, Marta (author)
Paris-Sorbonne University
Yi, Sukyoung K. (author)
Yonsei University
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 (creator_code:org_t)
2024
2024
English.
In: Astronomy and Astrophysics. - 0004-6361. ; 682
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The scaling relations between the gas content and star formation rate of galaxies provide useful insights into the processes governing their formation and evolution. We investigated the emergence and the physical drivers of the global Kennicutt-Schmidt (KS) relation at 0:25 ≤ z ≤ 4 in the cosmological hydrodynamic simulation NewHorizon, capturing the evolution of a few hundred galaxies with a resolution down to 34 pc. The details of this relation vary strongly with the stellar mass of galaxies and the redshift. A power-law relation ΣSFR / Σa gas with a ≈ 1:4, like that found empirically, emerges at z ≈ 2..3 for the more massive half of the galaxy population. However, no such convergence is found in the lower-mass galaxies, for which the relation gets shallower with decreasing redshift. At galactic scales, the star formation activity correlates with the level of turbulence of the interstellar medium, quantified by the Mach number, rather than with the gas fraction (neutral or molecular), confirming the conclusions found in previous works. With decreasing redshift, the number of outliers with short depletion times diminishes, reducing the scatter of the KS relation, while the overall population of galaxies shifts toward low densities. Our results, from parsec-scale star formation models calibrated with local Universe physics, demonstrate that the cosmological evolution of the environmental (e.g., mergers) and internal conditions (e.g., gas fractions) conspire to shape the KS relation. This is an illustration of how the interplay of global and local processes leaves a detectable imprint on galactic-scale observables and scaling relations.

Subject headings

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

Keyword

Galaxies: evolution
Galaxies: ISM
Galaxies: star formation
Methods: numerical
Turbulence

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