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. The air film pressure develops by hydrodynamic action as a result of the relative motion between the rotating part and the non-rotating top foil. Such bearings can either be journal bearings or thrust
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nucleosynthesis in violent episodes suffered by ancient stars" (with Dr Carolyn Doherty) "Applying 3D stellar hydrodynamics findings to 1D stellar codes: Improving the modelling of convection in stars" web page
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