Image Details
Caption: Figure 4.
Thickness change at the equator after spin-driven reshaping (Modification II). This quantity is equivalent to Δtr = (η − 1)χ(a0 + b0)/2. The contour plot shows Δtr in meters as a function of ejecta mass and speed. Positive values indicate that the axis on the equatorial plane widens owing to the described reshaping process.
© 2026. The Author(s). Published by the American Astronomical Society.