期刊
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
卷 57, 期 5, 页码 L39-L43出版社
OXFORD UNIV PRESS
DOI: 10.1093/pasj/57.5.L39
关键词
galaxy : center; ISM : clouds; ISM : jets and outflows; ISM : magnetic fields; magnetohydrodynamics : MHD simulation
We propose a new mechanism to explain the radio arc and threads in the Galactic center by current sheets produced by local magnetic shears due to the interaction of a moving cloud and a vertical field based on three-dimensional magnetohydrodynamical simulations. Magnetic reconnection and acceleration of cosmic-ray electrons in the current sheet would result in a high contrast of the radio emissivity inside and outside the arc and threads.
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