Image Details
Caption: Figure 6.
Top: upper limit of pressure (Equation (C1)) of dust aggregates below which monomer disruption can be neglected as a function of monomer radius. The blue and orange lines are for ice and silicate, whose material densities are 1.45 and 2.65 g cm−3, respectively. The parameters except for the material density are listed in Table 1. Bottom: upper limit of diameter of dust aggregates (Equation (C3)).
© 2024. The Author(s). Published by the American Astronomical Society.