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Modelling Planet Formation by Capture-Theory Interactions

Published online by Cambridge University Press:  26 May 2016

Michael M. Woolfson  and
Stephen Oxley
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
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 244 - 246
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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