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Ejection of substellar objects from accretion disks through stellar encounters
2015Stars often form in dense cluster environments, in which encounters between young stars are likely. If such an encounter happens while one of the stars has an extended disk that is gravitationally unstable, fragments formed within the disk can be ejected via multi-body gravitational interaction.
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Formation and Evolution of Minerals in Accretion Disks and Stellar Outflows
2003The contribution discusses dust formation and dust processing in oxygen rich stellar outflows under non-explosive conditions, and in circumstellar discs. The main topics are calculation of solid-gas chemical equilibria, the basic concepts for calculating dust growth under non-equilibrium conditions, dust processing by annealing and solid diffusion, a ...
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Deuterium-enriched water ties planet-forming disks to comets and protostars
Nature, 2023John J Tobin +2 more
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Diskoseismology: Signature of AGN and Stellar Mass Black Hole Accretion Disks
Annals of the New York Academy of Sciences, 1993R, Wagoner, M, Nowak
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Gravitational Instabilities in Circumstellar Disks
Annual Review of Astronomy and Astrophysics, 2016Kaitlin M Kratter, Giuseppe Lodato
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The building blocks of planets within the ‘terrestrial’ region of protoplanetary disks
Nature, 2004Michiel Min +2 more
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