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Kinematics of Galactic Centre clouds shaped by shear-seeded solenoidal turbulence

Petkova, Maya, 1990 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Kruijssen, J. M. D. (author)
Technische Universität München (TUM),Technical University of Munich (TUM)
Henshaw, Jonathan D. (author)
Liverpool John Moores University,Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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Longmore, S. (author)
Liverpool John Moores University
Glover, S. C.O. (author)
Ruprecht-Karls-Universität Heidelberg,Heidelberg University
Sormani, Mattia C. (author)
Ruprecht-Karls-Universität Heidelberg,Heidelberg University
Armillotta, Lucia (author)
Princeton University
Barnes, Ashley T. (author)
Universität Bonn,University of Bonn
Klessen, R. S. (author)
Ruprecht-Karls-Universität Heidelberg,Heidelberg University
Nogueras-Lara, Francisco (author)
European Southern Observatory (ESO)
Tress, Robin G. (author)
Armijos-Abendaño, Jairo (author)
Escuela Politécnica Nacional,Cardiff University
Colzi, L. (author)
Centro de Astrobiologia (CAB)
Federrath, C. (author)
Australian National University
Garcia, P. J.V. (author)
Universidad Catolica del Norte,Chinese Academy of Sciences
Ginsburg, A. (author)
University of Florida
Henkel, C. (author)
King Abdulaziz University,Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Martin, S. (author)
European Southern Observatory Santiago,Atacama Large Millimeter-submillimeter Array (ALMA)
Riquelme, D. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG),Universidad de La Serena,University of La Serena
Rivilla, Víctor M. (author)
Centro de Astrobiologia (CAB)
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 (creator_code:org_t)
2023
2023
English.
In: Monthly Notices of the Royal Astronomical Society. - 0035-8711 .- 1365-2966. ; 525:1, s. 962-968
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The Central Molecular Zone (CMZ; the central ∼500 pc of the Galaxy) is a kinematically unusual environment relative to the Galactic disc, with high-velocity dispersions and a steep size-linewidth relation of the molecular clouds. In addition, the CMZ region has a significantly lower star formation rate (SFR) than expected by its large amount of dense gas. An important factor in explaining the low SFR is the turbulent state of the star-forming gas, which seems to be dominated by rotational modes. However, the turbulence driving mechanism remains unclear. In this work, we investigate how the Galactic gravitational potential affects the turbulence in CMZ clouds. We focus on the CMZ cloud G0.253+0.016 ('the Brick'), which is very quiescent and unlikely to be kinematically dominated by stellar feedback. We demonstrate that several kinematic properties of the Brick arise naturally in a cloud-scale hydrodynamics simulation, that takes into account the Galactic gravitational potential. These properties include the line-of-sight velocity distribution, the steepened size-linewidth relation, and the predominantly solenoidal nature of the turbulence. Within the simulation, these properties result from the Galactic shear in combination with the cloud's gravitational collapse. This is a strong indication that the Galactic gravitational potential plays a crucial role in shaping the CMZ gas kinematics, and is a major contributor to suppressing the SFR, by inducing predominantly solenoidal turbulent modes.

Subject headings

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

Keyword

Galaxy: centre
stars: formation
ISM: kinematics and dynamics
galaxies: ISM
ISM: evolution
ISM: clouds

Publication and Content Type

art (subject category)
ref (subject category)

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