Equal-mass hyperbolic encounters in a uniform gas lose orbital energy, mostly lose eccentricity, and experience non-frictional forces that the standard Ostriker (1999) rectilinear model fails to capture.
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Gaseous Dynamical Friction on Hyperbolic Scatterings
Equal-mass hyperbolic encounters in a uniform gas lose orbital energy, mostly lose eccentricity, and experience non-frictional forces that the standard Ostriker (1999) rectilinear model fails to capture.