Maximum Galactic Disks vs. Hot Dark Halos
Astrophysics
2007-05-23 v1
Abstract
A 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.
Cite
@article{arxiv.astro-ph/0009041,
title = {Maximum Galactic Disks vs. Hot Dark Halos},
author = {Daniel Pfenniger},
journal= {arXiv preprint arXiv:astro-ph/0009041},
year = {2007}
}
Comments
5 pages, 1 figure, to appear in "Gas & Galaxy Evolution", VLA 20th Anniversary Conference, J.E. Hibbard, M.P. Rupen & J.H. van Gorkom (eds.)