Local simulations of common-envelope dynamical inspiral - Impact of rotation, accretion, and stratification

Open Access

Fig. 7.

Zoomed-in snapshots of the density at $t = 100 \tilde{R_{a}} / u_{\infty}$ $Mathematical equation: $ t = 100\,\widetilde{R_a}/u_{\infty} $$ , in the xy orbital plane (first panel) and on a spherical shell at radius r₂ (second panel).

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