A Resolution Requirement for Disk Simulations Modeling Collapse

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dc.creatorNelson, Andrew F.
dc.date2003-01-30
dc.date.accessioned2026-07-07T02:07:22Z
dc.date.available2026-07-07T02:07:22Z
dc.descriptionThe accurate simulation of collapsed objects requires that a huge range of spatial scales be well resolved if the result is not to be contaminated by numerically induced fragmentation. In this context, `insufficient resolution' means comparable to the local instability wavelength in the system. I define a minimum resolution criterion for simulations of disk systems, using the critical wavelength appropriate for disks.
dc.description4pages. Final version of submission for the "Scientific Frontiers in Research on Extrasolar Planets" conference: June 2002 in Washington
dc.identifierhttps://arxiv.org/abs/astro-ph/0301600
dc.identifierhttp://arxiv.org/abs/astro-ph/0301600
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5676
dc.subjectAstrophysics
dc.titleA Resolution Requirement for Disk Simulations Modeling Collapse
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