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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4 Pith papers cite this work, alongside 142 external citations. Polarity classification is still indexing.
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UNVERDICTED 4representative citing papers
Detection of a time-variable relativistic UV outflow at velocities up to 0.3c in quasar J2318, with estimated mass-loss rate and kinetic luminosity above typical feedback thresholds.
17-year Fermi-LAT observations detect GeV excesses in SS 433's W50 nebula whose spectra and positions suggest acceleration of cosmic-ray protons in microquasar outflows, potentially the first such evidence.
Deep VLBI observations of four ULXs yield no compact radio detections and tight upper limits, disfavoring persistently bright hard-state-like compact cores.
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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A New Member of the Fast and Furious Family: A Relativistic and Time-Variable UV Outflow in a Luminous Quasar
Detection of a time-variable relativistic UV outflow at velocities up to 0.3c in quasar J2318, with estimated mass-loss rate and kinetic luminosity above typical feedback thresholds.
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GeV emission around SS 433 with 17 years Fermi-LAT observation
17-year Fermi-LAT observations detect GeV excesses in SS 433's W50 nebula whose spectra and positions suggest acceleration of cosmic-ray protons in microquasar outflows, potentially the first such evidence.
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Deep VLBI constraints on compact radio cores in four ultraluminous X-ray sources
Deep VLBI observations of four ULXs yield no compact radio detections and tight upper limits, disfavoring persistently bright hard-state-like compact cores.