Hostname: page-component-7bb8b95d7b-pwrkn Total loading time: 0 Render date: 2024-09-18T15:41:11.785Z Has data issue: false hasContentIssue false
  • English
  • Français

Angular Momentum Transfer Due to Galactic Winds and Cooling Flows

Published online by Cambridge University Press:  25 May 2016

V. Missoulis
V. Missoulis*
Affiliation:
Astronomical Institute, National Observatory of Athens, P.O.Box 20048 - GR 11810 Athens - Greece

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We examine a model of galaxy formation where the bulge is formed at very early stages and this burst of star formation leads to a galactic wind which interacts with a huge surrounding gaseous envelope.

Type
Mergers & Remnants
Information
Symposium - International Astronomical Union , Volume 186: Galaxy Interactions at High and Low Redshift , 1999 , pp. 201
Copyright
Copyright © Kluwer 1999 

References

Missoulis, V. 1994, Astron. Reports, 38, 12 Google Scholar