Astronomy and Astrophysics – Astrophysics
Scientific paper
1994-06-02
Astronomy and Astrophysics
Astrophysics
plain TeX, PhD thesis, UC Berkeley 1993
Scientific paper
The formation of galaxies in hierarchical cosmogonies is studied using high resolution N-body plus SPH hydrodynamics simulations. The collapse of structure is followed self-consistently from Mpc scale filamentary structures to kpc scale galactic objects. The characteristics and formation processes of the galaxy like objects are studied in detail, along with the aggregation into a poor cluster. Related studies consider the effects of modelling star formation, the reliability of tracing galaxies in simulations, and tests of SPH methods. This submission serves first to notify that the full text and figures of my thesis are available in compressed PostScript form via anonymous ftp from astro.princeton.edu in the directory /summers/thesis (122 files, 19 MB compressed, 65 MB uncompressed). See the README file first. Second, this submission contains the title page, abstract, table of contents, introductory chapter, summary chapter, and references for my thesis. Those who are curious about the work may scan these pages to identify which chapters may be interesting to get via ftp.
No associations
LandOfFree
Cosmological Simulations of Galaxy Formation Including Hydrodynamics (hyper-abridged) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Cosmological Simulations of Galaxy Formation Including Hydrodynamics (hyper-abridged), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmological Simulations of Galaxy Formation Including Hydrodynamics (hyper-abridged) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-39342