MHD Simulation in Galactic Center Region with Radiative Cooling and Heating

We investigate the role of magnetic field on the gas dynamics in a galactic bulge region by three dimensional simulations with radiative cooling and heating. While high-temperature corona with $T>10^6\ {\rm K}$ is formed in the halo regions, the temperature near the mid-plane is $\lesssim 10^4\ {...

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Hauptverfasser:	Kakiuchi, Kensuke, Suzuki, Takeru. K, Inutsuka, Shu-ichiro, Inoue, Tsuyoshi, Shimoda, Jiro
Format:	Artikel
Sprache:	eng
Schlagworte:	Physics - Astrophysics of Galaxies Physics - High Energy Astrophysical Phenomena
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