Formation of galactic center magnetic loops

Mami Machida, Ryoji Matsumoto, Satoshi Nozawa, Kunio Takahashi, Yasuo Fukui, Natsuko Kudo, Kazufumi Torii, Hiroaki Yamamoto, Motosuji Fujishita, Kohji Tomisaka

Research output: Contribution to journalArticle

25 Citations (Scopus)

Abstract

A survey of the molecular clouds in the Galaxy with the NANTEN mm telescope has discovered molecular loops in the galactic center region. They show monotonic gradients of the line-of-sight velocity along the loops and large velocity dispersions towards their foot-points. It is suggested that these loops can be explained in terms of a buoyant rise of magnetic loops due to a Parker instability. We carried out global three-dimensional magneto-hydrodynamic simulations of the gas disk in the galactic center. The gravitational potential was approximated by an axisymmetric potential proposed by Miyamoto and Nagai (1975, PASJ, 27, 533). At the initial state, we assumed a warm (∼10 4K) gas torus threaded by azimuthal magnetic fields. Self-gravity and radiative cooling of the gas were ignored. We found that buoyantly rising magnetic loops are formed above the differentially rotating, magnetically turbulent disk. By analyzing the results of global MHD simulations, we identified individual loops, about 180 in the upper half of the disk, and studied their statistical properties, such as their length, width, height, and velocity distributions along the loops. The typical length and height of a loop are 1 kpc and 200 pc, respectively. The line-of-sight velocity changes linearly along a loop, and shows large dispersions around the foot-points. Numerical results indicate that loops emerge preferentially from the region where the magnetic pressure is large. We argue that these properties are consistent with those of molecular loops discovered by NANTEN.

Original languageEnglish
Pages (from-to)411-420
Number of pages10
JournalPublications of the Astronomical Society of Japan
Volume61
Issue number3
DOIs
Publication statusPublished - Jan 1 2009
Externally publishedYes

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gas
simulation
hydrodynamics
gravity
magnetic field
cooling
line of sight
gases
magnetohydrodynamic simulation
molecular clouds
gravitational fields
velocity distribution
telescopes
gravitation
galaxies
gradients
magnetic fields
distribution

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Machida, M., Matsumoto, R., Nozawa, S., Takahashi, K., Fukui, Y., Kudo, N., ... Tomisaka, K. (2009). Formation of galactic center magnetic loops. Publications of the Astronomical Society of Japan, 61(3), 411-420. https://doi.org/10.1093/pasj/61.3.411

Formation of galactic center magnetic loops. / Machida, Mami; Matsumoto, Ryoji; Nozawa, Satoshi; Takahashi, Kunio; Fukui, Yasuo; Kudo, Natsuko; Torii, Kazufumi; Yamamoto, Hiroaki; Fujishita, Motosuji; Tomisaka, Kohji.

In: Publications of the Astronomical Society of Japan, Vol. 61, No. 3, 01.01.2009, p. 411-420.

Research output: Contribution to journalArticle

Machida, M, Matsumoto, R, Nozawa, S, Takahashi, K, Fukui, Y, Kudo, N, Torii, K, Yamamoto, H, Fujishita, M & Tomisaka, K 2009, 'Formation of galactic center magnetic loops', Publications of the Astronomical Society of Japan, vol. 61, no. 3, pp. 411-420. https://doi.org/10.1093/pasj/61.3.411
Machida, Mami ; Matsumoto, Ryoji ; Nozawa, Satoshi ; Takahashi, Kunio ; Fukui, Yasuo ; Kudo, Natsuko ; Torii, Kazufumi ; Yamamoto, Hiroaki ; Fujishita, Motosuji ; Tomisaka, Kohji. / Formation of galactic center magnetic loops. In: Publications of the Astronomical Society of Japan. 2009 ; Vol. 61, No. 3. pp. 411-420.
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