Hostname: page-component-745bb68f8f-kw2vx Total loading time: 0 Render date: 2025-01-14T05:46:21.687Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Artymowicz, P. & Lubow, S. 1996, ApJ, in pressGoogle Scholar
Lin, & Papaloizou, , Protostars and Plants III, (1993), ed. Levy, & Lunine, , 749 Google Scholar
Sekiya, , Miyama, & Hayashi, , 1987, Earth Moon and Planets, 39, 1 Google Scholar