High resolution simulations of star formation

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dc.creatorBoffin, Henri M. J.
dc.creatorFrancis, Neil
dc.creatorWhitworth, Anthony P.
dc.date2001-10-09
dc.date.accessioned2026-07-07T02:00:43Z
dc.date.available2026-07-07T02:00:43Z
dc.descriptionIn order to study the capabilities of SPH in self-gravitating hydrodynamical problems, we have performed a series of three-dimensional numerical simulations of the collapse of a rotating homogeneous cloud, varying the number of particles and the artificial viscosity prescription.
dc.description2 pages, to appear in the proceedings of the IAU Symp. 208, "Astrophysical Supercomputing Using Particles", eds. J. Makino & P. Hut
dc.identifierhttps://arxiv.org/abs/astro-ph/0110198
dc.identifierhttp://arxiv.org/abs/astro-ph/0110198
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3501
dc.subjectAstrophysics
dc.titleHigh resolution simulations of star formation
dc.typetext

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