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Magnetic Activity in the Galactic Centre Region -- Fast Downflows along Rising Magnetic Loops
Kensuke Kakiuchi, Takeru K. Suzuki, Yasuo Fukui +4
We studied roles of the magnetic field on the gas dynamics in the Galactic bulge by a three-dimensional global magnetohydrodynamical simulation data, particularly focusing on verti…
Magnetohydrodynamic Simulations of the Formation of Molecular Clouds toward the Stellar Cluster Westerlund 2: Interaction of a Jet with Clumpy Interstellar Medium
Yuta Asahina, Tomohisa Kawashima, Naoko Furukawa +4
The formation mechanism of CO clouds observed with NANTEN2 and Mopra telescope toward the stellar cluster Westerlund 2 is studied by three-dimensional magnetohydrodynamic (MHD) sim…
Formation of Galactic Prominence in Galactic Central Region
Chih-Han Peng, Ryoji Matsumoto
We carried out 2.5-dimensional resistive MHD simulations to study the formation mechanism of molecular loops observed by Fukui et al. (2006) at Galactic central region. Since it is…
A Possible Time-Delayed Brightening of the Sgr A* Accretion Flow after the Pericenter Passage of G2 Cloud
Tomohisa Kawashima, Yosuke Matsumoto, Ryoji Matsumoto
A possibility of time-delayed radio brightenings of Sgr A* triggered by the pericenter passage of the G2 cloud is studied by carrying out global three-dimensional magnetohydrodynam…