Maximum Galactic Disks vs. Hot Dark Halos

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dc.creatorPfenniger, Daniel
dc.date2000-09-04
dc.date.accessioned2026-07-07T01:55:17Z
dc.date.available2026-07-07T01:55:17Z
dc.descriptionA series of arguments is presented for heavy galaxy disks not only in the optical regions, but also in the dark matter dominated regions of spirals. We are testing this possibility with extreme maximum disk N-body models without any conventional spheroidal dark halo.
dc.description5 pages, 1 figure, 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/0009041
dc.identifierhttp://arxiv.org/abs/astro-ph/0009041
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1603
dc.subjectAstrophysics
dc.titleMaximum Galactic Disks vs. Hot Dark Halos
dc.typetext

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