N-body simulations of warped galaxies

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dc.creatorRevaz, Yves
dc.creatorPfenniger, Daniel
dc.date2000-09-05
dc.date.accessioned2026-07-07T01:55:18Z
dc.date.available2026-07-07T01:55:18Z
dc.descriptionTwo methods generating warped galaxies with N-body simulations are presented. One uses an external potential as a disturber while the other is based on material accretion. The results of both methods are compared. A particular attention is given on the shape of the line of node (LON).
dc.description2 pages, to appear in "Gas & Galaxy Evolution", VLA 20th Anniversary Conference, J.E. Hibbard, M.P. Rupen & J.H. van Gorkom (eds.)
dc.identifierhttps://arxiv.org/abs/astro-ph/0009053
dc.identifierhttp://arxiv.org/abs/astro-ph/0009053
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1608
dc.subjectAstrophysics
dc.titleN-body simulations of warped galaxies
dc.typetext

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