Resolution requirements for simulating gravitational fragmentation using SPH

DOI10.1051/0004-6361:20054100zbMath1096.85003arXivastro-ph/0512247OpenAlexW3106402358WikidataQ68852205 ScholiaQ68852205MaRDI QIDQ5477368

D. A. Hubber, Anthony P. Whitworth, S. P. Goodwin

Publication date: 3 July 2006

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0512247

zbMATH Keywords

starsnumerical methodshydrodynamicsinstabilitiesformation

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

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