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We simulate the propagation of a shock front through the galactic halo induced by an explosion and/or a starburst at the galactic center. A huge dumbbell (Ω)-shaped shock front produced by an explosion of energy 3× 10⁵⁶ ergs about fifteen million years ago can mimic the radio and X-ray North Polar Spur as well the southern large X-ray spur. The post-shock high-temperature gas in the corona will explain the observed X-ray bulge around the galactic center. Key workds Galaxy: center -- Galaxy: halo -- Radio continuum: general -- Shock wave -- X-rays: general
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Yoshiaki Sofue (1994) studied this question.
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