Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...237...21v&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 237, no. 1, Oct. 1990, p. 21, 22.
Astronomy and Astrophysics
Astrophysics
6
Electron Density (Concentration), Galactic Cosmic Rays, Nucleon Potential, Starburst Galaxies, Energy Methods, Interstellar Gas, Interstellar Magnetic Fields
Scientific paper
An improved estimate of the nucleon-to-electron ratio in the cosmic ray
component of the starburst galaxy M 82 is presented. The ratio depends
on the filling factor for the hot gas. The minimum energy assumption for
calculating the magnetic field in M 82 is shown to be consistent with
the complete data set available for that galaxy.
Klein Ulf
Voelk Heinrich J.
Wielebinski Richard
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