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Modelling Planet Formation by Capture-Theory Interactions

Published online by Cambridge University Press:  26 May 2016

Michael M. Woolfson
Affiliation:
Physics Department, University of York, York, YO10 5DD, UK
Stephen Oxley
Affiliation:
Physics Department, University of York, York, YO10 5DD, UK

Abstract

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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
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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