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- W4214517245 abstract "The mechanisms of fragmentation of the equatorial dust disk around young stars and the formation of planetary systemsare considered. Using the model of librational motions of co-orbital asteroids of Jupiter, a model of viscous motion of gas,dust particles and small bodies in dust disks is constructed. The dynamic viscosity is obtained from the Navier-Stokesequation for three cases of characteristic flow orbits.It is shown that the librational orbits of Trojans at the early stages ofthe evolution of planetary systems could be transit orbits for dust particles during the formation of celestial bodies of smalland large sizes and masses." @default.
- W4214517245 created "2022-03-02" @default.
- W4214517245 creator A5074710593 @default.
- W4214517245 date "2022-02-22" @default.
- W4214517245 modified "2023-10-18" @default.
- W4214517245 title "Comparison of the dynamics of Jupiter’s coorbital asteroids and the dynamics of bodies in debris disks" @default.
- W4214517245 doi "https://doi.org/10.51194/vak2021.2022.1.1.018" @default.
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