Paper:	Numerical Simulations of Ringed Disk Galaxies
Volume:	197, XVth IAP Meeting Dynamics of Galaxies: From the Early Universe to the Present
Page:	11
Authors:	Buta, R.; Combes, F.
Abstract:	Near-infrared images are used to derive the gravitational potentials in three ringed barred disk galaxies: NGC 1433, 3081, and 6300. A sticky-particle dynamics code is used to evolve a cloud-particle disk in these potentials, and the resulting gaseous morphologies are compared with the observed strutures of the galaxies to deduce the bar pattern speed.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2025 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.038 seconds