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Molecular Loops in the Galactic Center. Yasuo Fukui Nagoya University. Molecular loops as evidence for magnetic floatation driven by Parker Instability. Magnetic loop in solar corona (TRACE : 191 Å ). Loop 1. 300 pc. 220 pc. MHD activities of galactic disks. Loop 2. 300 pc. 600 pc.
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Molecular Loops in the Galactic Center Yasuo Fukui Nagoya University
Molecular loops as evidence for magnetic floatation driven by Parker Instability Magnetic loop in solar corona (TRACE:191Å) Loop 1 300 pc 220 pc MHD activities of galactic disks Loop 2 300 pc 600 pc Fukui et al. (2006)
-150 km/s -70 km/s -110 km/s -50 km/s Velocity distributions of the loops Loop 2 Loop 1 Torii et al. (2009a), submitted
Position-Velocity diagram (range b = 0.5 – 2.5°) Color:12CO Contour:13CO(white) Fukui et al. (2006)
Magnetic loops in the GC Machida et al. (2009) NANTEN CO(J=1-0) 20-200 km/s ・ MHD numerical calculation found a number of loops in the Galactic center ・ Fujishita et al. (2009) discovered loop 3.
CO vs HI color:HI(Parkes), contours:CO(NANTEN) 3kpc - arm H2 mass: loop 1 = 2×105 Msun, loop 2 = 3×105 Msun HI mass:loop 1 = 2×105 Msun, loop 2 = 3×105 Msun → Total Ek ~ 1052 erg
Helix like distributions in the loops Color: CO(2-1) NANTEN2Contour : CO(1-0) NANTEN
Formation of the helix components Helix on the Sun Shibata & Matsumoto 1991 • A helical magnetic field could be formed by… • Shear motion by differential rotation. • Coriolis force for floating loops. (Shibata & Matsumoto 1991) • ・ Kink instability amplifies the degree of distortion
Foot point in 12CO(J=3-2) ASTE CO(J=3-2) -180 - -40 km/s NANTEN CO(J=1-0)
12CO(J=3-2) VB diagram • U shape • Broad emissions • Protrusion
12CO(J=3-2)/12CO(J=1-0) ratio: R3-2/1-0 Color:R3-2/1-0, Contours:ASTE CO(J=3-2)
LVG result R3-2/1-0 VB diagram Tk ~ 90 K
U shape Isobe et al. 2007 Isobe et al. (2007) • Down flow from two loops forms U shape in both space and velocity. • Magnetic reconnection may occur at the foot point.