2000/09/04 by D. Pfenniger, Daniel Pfenniger, Pfenniger, Daniel
Physics and Astronomy · #Astronomy and Astrophysical Research #Galaxies: Formation, Evolution, Phenomena #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0009041
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.)
arxiv created 2000/09/04 · arxiv updated 2009/12/01
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.