In global common-envelope simulations, drag on the companion after the first periastron is up to an order of magnitude below Bondi-Hoyle-Lyttleton predictions and depends only weakly on companion mass.
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How Drag Force Evolves in Global Common Envelope Simulations
In global common-envelope simulations, drag on the companion after the first periastron is up to an order of magnitude below Bondi-Hoyle-Lyttleton predictions and depends only weakly on companion mass.