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An SPH code for galaxy formation problems - Presentation of the code
Uppsala University.
Uppsala University.
1997 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 324, no 2, 534-548 p.Article in journal (Other scientific) Published
Abstract [en]

We present and test a code for two-fluid simulations of galaxy formation, one of the fluids being collision-less. The hydrodynamical evolution is solved through the SPH method while gravitational forces are calculated using a tree method. The code is Lagr

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1997. Vol. 324, no 2, 534-548 p.
Keyword [en]
hydrodynamics; numerical methods; galaxies: formation; SMOOTHED PARTICLE HYDRODYNAMICS; N-BODY SYSTEMS; SIMULATIONS; DYNAMICS
URN: urn:nbn:se:uu:diva-85339OAI: oai:DiVA.org:uu-85339DiVA: diva2:113247
Addresses: Hultman J, ASTRON OBSERV, BOX 515, S-75120 UPPSALA, SWEDEN.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-15

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