Image Details
Caption: Figure 2.
The eccentricity growth rate (upper panel) and precession rate (lower panel) as a function of H/r are shown for various disk outer radii and q = 0.1. The dotted lines show the solution to the 2D equations, and the solid lines show the solution to the 3D equations.
© 2026. The Author(s). Published by the American Astronomical Society.