Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.atnf.csiro.au/pasa/16_1/nulsen/paper/index.html
Дата изменения: Fri Apr 8 08:53:52 2016
Дата индексирования: Sun Apr 10 15:43:37 2016
Кодировка:

Поисковые слова: rainbow
Gas and Galaxy Formation

Gas and Galaxy Formation

P.E.J. Nulsen, PASA, 16 (1), 3
The html and gzipped postscript versions of this paper are in preprint form.
To access the final published version, download the pdf file
.



Next Section: Introduction
Contents Page: Volume 16, Number 1

Gas and Galaxy Formation

P.E.J. Nulsen 1

1 Department of Engineering Physics, University of Wollongong, Wollongong, NSW 2522, Australia
EMAIL pejn@uow.edu.au

Abstract:

The theory of galaxy formation is reviewed briefly. From the evidence of clusters today, the primordial gas fraction was 20 percent or more. Thus, while the Universe is dominated by dark matter, gas plays an appreciable role in galaxy formation. Collapses of dwarf protogalaxies produce predominantly cold gas. It is argued that, in such cold collapses, the collapsed gas is largely self-gravitating. As a result, gas processes play a critical role in determining the visible structure of galaxies.

Keywords: galaxies: formation





Welcome... About Electronic PASA... Instructions to Authors
ASA Home Page... CSIRO Publishing PASA
Browse Articles HOME Search Articles
б© Copyright Astronomical Society of Australia 1997
ASKAP
Public