CO observations reveal molecular clumps at SS 433 X-ray jet re-brightening sites, providing evidence that jet-cloud shocks enhance nonthermal X-ray emission via turbulence and magnetic field amplification.
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2D RMHD simulations show recollimation distance decreases monotonically with magnetization σ, converging to z_MHD/z_HD ∝ (B₀²/P_ext)^{-1/3} in the high-σ regime, with toroidal fields producing localized emission knots and poloidal fields shifting the zone downstream.
citing papers explorer
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Discovery of CO Clouds Associated with the X-ray Jets of SS 433: Evidence for Shock-Cloud Interaction Enhancing Nonthermal X-ray Emission
CO observations reveal molecular clumps at SS 433 X-ray jet re-brightening sites, providing evidence that jet-cloud shocks enhance nonthermal X-ray emission via turbulence and magnetic field amplification.
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2D magnetohydrodynamic jet simulations: properties of recollimation shocks
2D RMHD simulations show recollimation distance decreases monotonically with magnetization σ, converging to z_MHD/z_HD ∝ (B₀²/P_ext)^{-1/3} in the high-σ regime, with toroidal fields producing localized emission knots and poloidal fields shifting the zone downstream.