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Wiley InterScience

Astronomy & Geophysics

Astronomy & Geophysics

Volume 46 Issue 6, Pages 6.28 - 6.33

Published Online: 30 Nov 2005

© 2010 Royal Astronomical Society



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Barred galaxies
Stars and bars
Johan H Knapen 1
  1 Professor of Astronomy at the University of Hertfordshire

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

ABSTRACT

Bars 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

AbstractBars as long-lived featuresMovements of stars and gas in barsEffects of bars: gas inflowFuture prospectsNumerical modellingFurther reading

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.


DIGITAL OBJECT IDENTIFIER (DOI)
10.1111/j.1468-4004.2005.46628.x About DOI

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