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Highlights of Astronomy
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Highlights of Astronomy
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Magnetic Fields in Irregular Galaxies

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 2002 English Publisher:Cambridge University Press (CUP)Journal:Highlights of Astronomy, volume 12, pages 721-722 (issn: 1539-2996, Copyright policy )
Authors: Krzysztof T. Chyzy;

doi: 10.1017/s1539299600014775

Magnetic Fields in Irregular Galaxies

Abstract

AbstractRadio data of large irregular galaxies reveal some extended synchrotron emission with a substantial degree of polarization. In the case of NGC 4449 strong galaxy-scale regular magnetic fields were found, in spite of the lack of ordered rotation required for the conventional dynamo action. The rigidly rotating large irregular NGC 55 shows vertical polarized spurs connected with a network of ionized gas filaments. Small dwarf irregulars show only isolated polarized spots.

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
1
Average
Average
Average
bronze
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