Dark matter in low mass surface density galaxies

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dc.creatorChemin, Laurent
dc.creatorCarignan, Claude
dc.creatorAmram, Philippe
dc.date2007-07-10
dc.date.accessioned2026-07-07T08:14:54Z
dc.date.available2026-07-07T08:14:54Z
dc.descriptionLow mass surface density spiral and irregular galaxies like low surface brightness (LSB) and dwarf galaxies are unique laboratories to study the dynamical properties of Dark Matter halos because their mass is generally dominated by dark matter at all galactocentric radii. We present results from the largest sample ever assembled of high resolution Halpha velocity fields of LSB and dwarf galaxies in order to study their mass distributions.
dc.description2 pages, 1 figure, proceedings of the conference "Pathways Through an Eclectic Universe", Johan Knapen, Terry Mahoney, and Alexandre Vazdekis eds
dc.identifierhttps://arxiv.org/abs/0707.1479
dc.identifierhttp://arxiv.org/abs/0707.1479
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/133294
dc.subjectAstrophysics
dc.titleDark matter in low mass surface density galaxies
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