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Wiley InterScience | ||||||||||
![]() Astronomy & GeophysicsVolume 46 Issue 6, Pages 6.28 - 6.33 Published Online: 30 Nov 2005 © 2010 Royal Astronomical Society Published on behalf of the Royal Astronomical Society
Abstract | References | Full Text: HTML, PDF (Size: 424K) | Related Articles | Citation Tracking Barred galaxies Stars and bars He acknowledges support from the Leverhulme Trust in the form of a Leverhulme Research Fellowship, and comments on an earlier form of the manuscript from J E Beckman and I Shlosman. Copyright Royal Astronomical Society ABSTRACTBars are a common feature of disc galaxies and, as such, must be taken into account in understanding the evolution of structure within galaxies, argues Johan H Knapen. Abstract
Bars are prominent features that occur in most disc galaxies and have important dynamical effects on their hosts. This paper describes some of the known properties of bars, illustrating the discussion with images that show the beauty of the galaxies under consideration. The focus of this article is on the evolution of bars and on their influence on the redistribution of matter within galaxies. In this way, bars drive the internal, or secular, evolution of galaxies. |