Image Details
Caption: Figure 5.
Scale-height modulation factor λH obtained by solving Equation (30) (λH,OL, left) and from the simulations (﹩{\lambda }_{H,{\rm{sim}}}﹩, right) for ﹩{\dot{M}}_{{\rm{in}}}=1{0}^{-7}\,{M}_{\odot }\,{{\rm{yr}}}^{-1}﹩ (top) and 10−6 M⊙ yr−1 (bottom) at t = 28 kyr. The simulated scale-height variations agree well with those predicted by the analytic framework of G. I. Ogilvie & E. M. Lynch (2019).
© 2026. The Author(s). Published by the American Astronomical Society.