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SPH Simulations of Protoplanetary Perturbers in Gas Disks

Published online by Cambridge University Press:  12 April 2016

Sarah Maddison  and
Pierre Barge
Sarah Maddison
Affiliation:
Mathematics Department, Monash University, Clayton, 3168, Australia
Pierre Barge
Affiliation:
Laboratoire d’Astronomie Spatiale, BP 8, Marseille, 13376, France

Abstract

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We use Smoothed Particle Hydrodynamics (SPH) to numerically investigate gap clearing around a protoplanetary body in a selfgravitating gaseous disk. It has been suggested that proto-Jupiter regulated it’s own growth by clearing a gap around itself and thus halting accretion.

Type
Part 15. Poster Papers
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 758 - 759
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

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