Simulations of Galaxy Formation in Hierarchically Clustering Universes
Abstract
Description
I review the results of recent N--body/hydrodynamical simulations of the formation of galaxies in hierarchical universes, with special emphasis on the structure of dark matter halos, as well as on the mass and angular momentum of gaseous disks that assemble at the center of these halos.
compressed and uuencoded PS file with no figures. 73095 bytes. Compressed PS file (10 pages including 5 figures) available by anonymous ftp from ftp://penedes.as.arizona.edu/pub/jfn/papers/iap95/iap95.ps.Z . Invited Review to be published in the Proceedings of the 11th IAP Meeting, 'The Interplay between Massive Star Formation, the ISM and Galaxy Evolution', eds. D. Kunth et al. (Paris:Editions Frontieres)
compressed and uuencoded PS file with no figures. 73095 bytes. Compressed PS file (10 pages including 5 figures) available by anonymous ftp from ftp://penedes.as.arizona.edu/pub/jfn/papers/iap95/iap95.ps.Z . Invited Review to be published in the Proceedings of the 11th IAP Meeting, 'The Interplay between Massive Star Formation, the ISM and Galaxy Evolution', eds. D. Kunth et al. (Paris:Editions Frontieres)