HIGHLIGHTS
- who: Du00f6rner Julien and collaborators from the Ruhr-Universitu00e4t Bochum, Theoretische Physik IV: Plasma-Astroteilchenphysik, Universitu00e4tsstrau00dfe, Bochum, Germany University of Hamburg, Hamburger Sternwarte, Gojenbergsweg, Hamburg, Germany have published the Article: Cosmic-ray electron transport in the galaxy M, in the Journal: (JOURNAL)
- what: Diff/ adv time scale [Myr] lines) at the edge of the galaxy is due to the vanishing magnetic_field strength in the outer part (see Fig 1).
- how: The height of the disc is considered to be hd=3 kpc and for the magnetic_field height the authors used hb=6 kpc . . .
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