Preprint
Star Formation, Supernovae Feedback and the Angular Momentum Problem in Numerical CDM Cosmogony: Half Way There?
Abstract
We present a smoothed particle hydrodynamic (SPH) simulation that reproduces
a galaxy that is a moderate facsimile of those observed. The primary failing
Authors
Thacker RJ; Couchman HMP
Publication date
June 4, 2001
DOI
10.48550/arxiv.astro-ph/0106060
Preprint server
arXiv