Motion properties of satellites around external spiral galaxies

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dc.creatorAzzaro, M.
dc.creatorPrada, F.
dc.creatorGutiérrez, C. M.
dc.date2003-10-17
dc.date.accessioned2026-07-07T02:10:34Z
dc.date.available2026-07-07T02:10:34Z
dc.descriptionWe are analyzing a sample of closeby galaxy systems, each comprising a bright isolated spiral and its satellites. We find an excess (56%) of prograde satellites over retrograde, which basically holds for all angular displacements from the primary major axis. Monte Carlo simulations show that interlopers and mixing systems at different distances in the sample should not affect porcentages sensibly.
dc.description4 pages, 1 figure, proceedings of the conference "Satellites and tidal streams"
dc.identifierhttps://arxiv.org/abs/astro-ph/0310487
dc.identifierhttp://arxiv.org/abs/astro-ph/0310487
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6777
dc.subjectAstrophysics
dc.titleMotion properties of satellites around external spiral galaxies
dc.typetext

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