Home ContactSitemap CAS中文
About Us
Brief Introduction
History
Directors
Organization
Research Groups
Scientific Progress
Seminars
Colloquia
CAS Members
Experts
Faculty
Research Fields
Center for Astro-geodynamics
Astrophysics Division
DRAST (Division of Radio Astronomy Science and Technology )
High Technology Laboratories

Location: Home>Research>Seminars
Gaseous Substructures in Barred Galaxies
Author:
ArticleSource:
Update time: 2012-07-26
Close
Text Size: A A A
Print

  Title: Gaseous Substructures in Barred Galaxies
   Speaker: Woong-Tae Kim (Seoul National University)
   Time: 2012, July 26 (Thursday), 2pm
   Location: middle conference room

Abstract:
  tract:The inner parts of barred galaxies contain interesting gaseous substructures that include dust lanes, nuclear rings, and nuclear spirals. Understanding their formation and evolution is of crucial importance to understand how the interstellar gas in barred galaxies is driven inward to affect star formation activities in the nuclear regions.  Since the gas flows shaping them are highly nonlinear, numerical simulations have been an indispensable tool to study their formation, evolution, and associated dynamics.  In this talk, I will present recent results of our high-resolution simulations, focusing on the effects of bar strength and magnetic fields on the properties of
  bar substructures and star formation occurring in nuclear rings.  I will also discuss the numerical results in comparison with observations.

Shanghai Astronomical Observatory, All Rights Reserved
80 Nandan Road, Shanghai 200030, China
Tel: +86-21-64386191 Email:shao@shao.ac.cn