Magnetic field morphology and evolution in the Central Molecular Zone and its effect on gas dynamics
Artikel i vetenskaplig tidskrift, 2024

The interstellar medium in the Milky Way's Central Molecular Zone (CMZ) is known to be strongly magnetised, but its large-scale morphology and impact on the gas dynamics are not well understood. We explore the impact and properties of magnetic fields in the CMZ using three-dimensional non-self gravitating magnetohydrodynamical simulations of gas flow in an external Milky Way barred potential. We find that: (1) The magnetic field is conveniently decomposed into a regular time-averaged component and an irregular turbulent component. The regular component aligns well with the velocity vectors of the gas everywhere, including within the bar lanes. (2) The field geometry transitions from parallel to the Galactic plane near z = 0 to poloidal away from the plane. (3) The magneto-rotational instability (MRI) causes an in-plane inflow of matter from the CMZ gas ring towards the central few parsecs of 0.01-0.1 M· yr-1 that is absent in the unmagnetised simulations. However, the magnetic fields have no significant effect on the larger-scale bar-driven inflow that brings the gas from the Galactic disc into the CMZ. (4) A combination of bar inflow and MRI-driven turbulence can sustain a turbulent vertical velocity dispersion of Ï∼ = 5 km s-1 on scales of 20 pc in the CMZ ring. The MRI alone sustains a velocity dispersion of Ï ∼ 3 km s-1. Both these numbers are lower than the observed velocity dispersion of gas in the CMZ, suggesting that other processes such as stellar feedback are necessary to explain the observations. (5) Dynamo action driven by differential rotation and the MRI amplifies the magnetic fields in the CMZ ring until they saturate at a value that scales with the average local density as Ba 102 (n/103 cm-3)0.33 μG. Finally, we discuss the implications of our results within the observational context in the CMZ.

Galaxy: kinematics and dynamics

Galaxy: center

ISM: magnetic fields

Författare

Robin G. Tress

Observatoire de Sauverny

Mattia C. Sormani

University of Surrey

Universita degli Studi dell'Insubria

P. Girichidis

Universität Heidelberg

S. C.O. Glover

Universität Heidelberg

R. S. Klessen

Universität Heidelberg

R. Smith

University of Manchester

University of St Andrews

E. Sobacchi

Istituto nazionale di astrofisica (INAF)

Lucia Armillotta

Princeton University

Ashley T. Barnes

European Southern Observatory (ESO)

C. Battersby

University of Connecticut

K. R.J. Bogue

University of Manchester

N. Brucy

Universität Heidelberg

L. Colzi

Centro de Astrobiologia (CAB)

C. Federrath

Australian National University

ARC Centre of Excellence for All-sky Astrophysics

P. García

Universidad Catolica del Norte

Chinese Academy of Sciences

A. Ginsburg

College of Liberal Arts and Sciences

J. Göller

Universität Heidelberg

H. P. Hatchfield

University of Connecticut

California Institute of Technology (Caltech)

C. Henkel

Max-Planck-Gesellschaft

P. Hennebelle

Université Paris-Saclay

Jonathan D. Henshaw

Liverpool John Moores University

Max-Planck-Gesellschaft

Michaela Hirschmann

Osservatorio Astronomico di Trieste

Observatoire de Sauverny

Y. Hu

University of Wisconsin Madison

J. K. F. Mann

Massachusetts Institute of Technology (MIT)

J.M. Diederik Kruijssen

COOL Research DAO

Technische Universität München

A. Lazarian

University of Wisconsin Madison

D. Lipman

University of Connecticut

S. Longmore

COOL Research DAO

Liverpool John Moores University

M. R. Morris

University of California

Francisco Nogueras-Lara

European Southern Observatory (ESO)

Maya Petkova

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

T. Pillai

Massachusetts Institute of Technology (MIT)

Víctor M. Rivilla

Centro de Astrobiologia (CAB)

A. Sanchez-Monge

Consejo Superior de Investigaciones Científicas (CSIC)

Centre Tecnològic de Telecomunicacions de Catalunya (CTTC)

J. D. Soler

Istituto nazionale di astrofisica (INAF)

D. Whitworth

Universidad Nacional Autónoma de México

Universität Heidelberg

Q. Zhang

Harvard-Smithsonian Center for Astrophysics

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 691 A303

Ämneskategorier (SSIF 2011)

Astronomi, astrofysik och kosmologi

DOI

10.1051/0004-6361/202450035

Mer information

Senast uppdaterat

2025-03-09