Results 81 to 90 of about 399,848 (263)
Accumulation of Dust on a Surface and the Subsequent Formation of Compact Aggregate Piles
Abstract Dust aggregation is a prominent topic in space physics, yet the accumulation of dust on surfaces in airless environments remains poorly understood. It is commonly assumed that, during the initial stages of dust deposition, particles spread uniformly to form a monolayer.
G. Griffin +4 more
wiley +1 more source
We introduce Disk2Planet, a machine-learning-based tool to infer key parameters in disk–planet systems from observed protoplanetary disk structures. Disk2Planet takes as input the disk structures in the form of 2D density and velocity maps, and outputs ...
Shunyuan Mao +5 more
doaj +1 more source
Dust Size Growth and Settling in a Protoplanetary Disk
We have studied dust evolution in a quiescent or turbulent protoplanetary disk by numerically solving coagulation equation for settling dust particles, using the minimum mass solar nebular model.
Hideko Nomura +12 more
core +1 more source
Abstract It has been proposed that IIE iron meteorites formed through impact processes on a parent body that was composed of either the H chondrites or a much‐debated fourth ordinary chondrite group, the HH chondrites. To resolve this debate, we have compiled a large dataset for the ordinary chondrites, low‐fayalite ungrouped chondrites, and IIE irons,
Rachel S. Kirby +2 more
wiley +1 more source
Shadows, gaps, and ring-like structures in protoplanetary disks [PDF]
We study the structure of passively heated disks around T Tauri and Herbig Ae stars, and present a vectorized Monte Carlo dust radiative transfer model of protoplanetary disks. The vectorization provides a speed up factor of 100 when compared to a scalar
Acke +104 more
core +2 more sources
disksurf: Extracting the 3D Structure of Protoplanetary Disks [PDF]
Richard Teague +3 more
openalex +1 more source
Close binary systems present challenges to planet formation. As binary separations decrease, so do the occurrence rates of protoplanetary disks in young systems and planets in mature systems.
Benjamin M. Tofflemire +10 more
doaj +1 more source
In this chapter, we cover the formation of protoplanetary disk as a natural byproduct of the gravitational collapse of a slowly rotating, hydrostatic cloud.
Dominik Carsten
doaj +1 more source
The Structure and Evolution of Protoplanetary Disks: an infrared and submillimeter view
Circumstellar disks are the sites of planet formation, and the very high incidence of extrasolar planets implies that most of them actually form planetary systems.
Cieza, Lucas A.
core +1 more source
Simulation of Thermal Surface Waves in a Protoplanetary Disk in a Two-Dimensional Approximation [PDF]
Ya. N. Pavlyuchenkov +2 more
openalex +1 more source

