Interplay of CR-driven galactic wind, magnetic field, and galactic dynamo in spiral galaxies
2008 ◽
Vol 4
(S259)
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pp. 547-548
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AbstractFrom our radio observations of the magnetic field strength and large-scale pattern of spiral galaxies of different Hubble types and star formation rates (SFR) we conclude that – though a high SFR in the disk increases the total magnetic field strength in the disk and the halo – the SFR does not change the global field configuration nor influence the global scale heights of the radio emission. The similar scale heights indicate that the total magnetic field regulates the galactic wind velocities. The galactic wind itself may be essential for an effective dynamo action.
2012 ◽
Vol 10
(H16)
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pp. 399-399
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1990 ◽
Vol 140
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pp. 233-234
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2012 ◽
Vol 10
(H16)
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pp. 615-615
2010 ◽
Vol 725
(1)
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pp. 1306-1316
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2008 ◽
Vol 4
(S259)
◽
pp. 109-110
2010 ◽
Vol 6
(S271)
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pp. 187-196
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