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Southern eROSITA bubble as a forward shock and the low-metallicity CGM. South-east side story

Churazov, E. et al.
arXiv (OAI Expanded) · Papers
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astrophysics-of-galaxieshigh-energy-astrophysical-phenomena
Unlike the complicated X-ray and radio structure observed in the North Polar Spur area, the South-Eastern part of the eROSITA bubbles can be reasonably well described as a propagating forward shock, plausibly created by the transient energy release at the Galactic Center. In this model, the physical
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