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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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.