4 citations · 7 across the 3 of their papers we have counts for
3 papers
physics.space-ph2004
Gravitational Interactions Between Protoplanets and Planetismal Disks of Equal Mass
B. D. Lindsay, K. W. Orr, T. W. Hyde +1
Numerical simulations show that planetesimal systems with unevenly distributed masses may actually be more stable than those where all the bodies are of roughly equal size.
physics.space-ph2003★ 3 cited
Dust Grain Orbital Behavior Around Ceres
R. Nazzario, T. W. Hyde, L. Barge
Many asteroids show indications they have undergone impacts with meteoroid particles having radii between 0.01 m and 1 m. During such impacts, small dust grains will be ejected at…
physics.space-ph2003★ 4 cited
Finite Coulomb Crystal Formation
J. Vasut, T. W. Hyde, L. Barge
Dust particles immersed within a plasma environment, such as those found in planetary rings or comets, will acquire an electric charge. If the ratio of the inter-particle potential…