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The Violent Interstellar Medium of Nearby Dwarf Galaxies

Published online by Cambridge University Press:  05 March 2013

Fabian Walter
Fabian Walter*
Affiliation:
Radioastronomisches Institut, Auf dem Hügel 71, 53121 Bonn, Germany; walter@astro.uni-bonn.de
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Abstract

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High resolution HI observations of nearby dwarf galaxies (most of which are situated in the M81 group at a distance of about 3·2 Mpc) reveal that their neutral interstellar medium (ISM) is dominated by hole-like features most of which are expanding. A comparison of the physical properties of these holes with the ones found in more massive spiral galaxies (such as M31 and M33) shows that they tend to reach much larger sizes in dwarf galaxies. This can be understood in terms of the galaxy's gravitational potential. The origin of these features is still a matter of debate. In general, young star forming regions (OB-associations) are held responsible for their formation. This picture, however, is not without its critics and other mechanisms such as the infall of high velocity clouds, turbulent motions or even gamma ray bursters have been recently proposed. Here I will present one example of a supergiant shell in IC 2574 which corroborates the picture that OB associations are indeed creating these structures. This particular supergiant shell is currently the most promising case to study the effects of the combined effects of stellar winds and supernova explosions which shape the neutral interstellar medium of (dwarf) galaxies.

Keywords

galaxies: individual (IC 2574, Holmberg II, DDO 47, NGC 3077)ISM: kinematic and dynamicsISM: structure radio linesISM: X-rays

Information

Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 16 , Issue 1 , 1999 , pp. 106 - 112
Copyright
Copyright © Astronomical Society of Australia 1999

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