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Using radio polarimetry we study the connection between the transport of cosmic rays (CR's), the three-dimensional magnetic field structure, and features of other ISM phases in the halo of NGC 253.
F. Krause & R. Beck, Symmetry and direction of seed magnetic fields in galaxies , A&A , 335
1998
Earlier work this paper cites.
R. Beck & M. Krause, Revised equipartition and minimum energy formula for magnetic field strength estimates from radio synchrotron observations , Astr. Nachr. , 326
2005
Earlier work this paper cites.
V. Heesen, Cosmic rays and the magnetic field in the nearby starburst galaxy NGC 253 , PhD thesis , Ruhr-University Bochum, Germany (2008)
2008
Cited alongside, same era.
V. Heesen, R. Beck, M. Krause, & R.-J. Dettmar, Cosmic rays and the magnetic field in the nearby starburst galaxy NGC 253 I. The cosmic ray distribution , A&A (2008), in prep
2008
Cited alongside, same era.
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