Image Details
                    Caption: Figure 4.
Same as the left panel of Figure 3, but showing the evolution in the T vs. Σ plane as the value of the collision/ablation-heating parameter β is increased at constant logarithmic intervals between 10−3 and 0.25 (as labeled in color). The thermally stable solution obtained for β = 0.25 > β stable = 3/16 is indicated by a red star.
© 2024. The Author(s). Published by the American Astronomical Society.