Predicting Dust Distribution in Protoplanetary Discs

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dc.creatorBarriere-Fouchet, Laure
dc.creatorGonzalez, Jean-Francois
dc.creatorHumble, Robin J.
dc.creatorMaddison, Sarah T.
dc.creatorMurray, James R.
dc.date2003-10-31
dc.date.accessioned2026-07-07T02:10:59Z
dc.date.available2026-07-07T02:10:59Z
dc.descriptionWe present the results of three-dimensional numerical simulations that include the effects of hydrodynamical forces and gas drag upon an evolving dusty gas disk. We briefly describe a new parallel, two phase numerical code based upon the smoothed particle hydrodynamics (SPH) technique in which the gas and dust phases are represented by two distinct types of particles. We use the code to follow the dynamical evolution of a population of grains in a gaseous protoplanetary disk in order to understand the distribution of grains of different sizes within the disk. Our ``grains'' range from metre to submillimetre in size.
dc.description2 pages, LaTeX with 1 ps figure embedded, using newpasp.sty (supplied). To appear in the proceedings of the XIXth IAP colloquium "Extrasolar Planets: Today and Tomorrow" held in Paris, France, 2003, June 30 -- July 4, ASP Conf. Ser
dc.identifierhttps://arxiv.org/abs/astro-ph/0310909
dc.identifierhttp://arxiv.org/abs/astro-ph/0310909
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6924
dc.subjectAstrophysics
dc.titlePredicting Dust Distribution in Protoplanetary Discs
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