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Modelling Planet Formation by Capture-Theory Interactions
Published online by Cambridge University Press: 26 May 2016
Abstract
Diffuse low-mass stars and brown dwarfs coexist with condensed solar-type stars in the embedded stage of a developing open cluster. It is shown by smoothed-particle-hydrodynamics modelling that interactions between stars and protostars leads to disruption of the protostar to form protoplanets that can then be captured by the star.
- Type
- Part II: Progress in the theory of planet formation
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- Copyright © Astronomical Society of the Pacific 2004