Titlebook: Galactic and Intergalactic Magnetic Fields; Ulrich Klein,Andrew Fletcher Book 2015 Springer International Publishing Switzerland 2015 Astr

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Sander Happaerts,Hans Bruyninckxstic electrons moving in a magnetic field for which there is other independent evidence (Sect. .), this radiation turns out to be the main diagnostic tool to trace magnetic fields in interstellar and intergalactic space, by virtue of its radiation spectrum and polarisation characteristics.

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flaggy

Erwan Josse,Pascal Bach,Laurent Dagornential made up by stars and dark matter. In spiral galaxies, the gas has a neutral and an ionised phase. The neutral phase is made up by (in order of decreasing density) the molecular medium, the cold neutral medium (CNM), and the warm neutral medium (WNM). The ionised phase consists of the warm (WI

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C. Bardos,F. Golse,D. Levermoreer a solid understanding of the basic ideas of galactic dynamo theory, which will allow them to engage with current research in this active field. To begin, we use qualitative arguments to derive a very simple mathematical model for a dynamo that includes some of the key elements of dynamo theory. T

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collagenase

Knowledge Database and Inversionich are dwarf galaxies. For example, the Virgo Cluster contains some 250 large galaxies and more than 2000 smaller ones. Small assemblies of galaxies are referred to as groups. For instance, the local group comprises two really massive galaxies, the Milky Way and M 31, and a third one, M 33, being s

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J. Tiago Gonçalves,Ricardo MostanyIn this chapter, we shall treat the main diagnostic tools that we have at hand to investigate interstellar and intergalactic magnetic fields.

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