Implications of the unification of cosmic ray transport and Galactic wind models

Details Implications of the unification of cosmic ray transport and Galactic wind models Implications of the unification of cosmic ray transport and Galactic wind models

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...239..424p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 239, no. 1-2, Nov. 1990, p. 424-436.

Astronomy and Astrophysics

Astronomy

11

Galactic Cosmic Rays, Galactic Radio Waves, Solar Wind, Transport Properties, Continuous Radiation, Diffusion Coefficient, Galactic Radiation, Radio Astronomy

Scientific paper

A first approach is presented to the unification of cosmic ray transport models and those for the gas dynamics in a Galactic wind. Using a previously derived solution of a steady-state transport equation where the electrons undergo simultaneous diffusion, convection, adiabatic deceleration, radiative losses, and injection, the corresponding synchrotron line-of-sight integrals are solved. The results are applied to a hydrodynamical model for a Galactic wind to describe the spatial variations of important parameters and especially the spatial variations of some synchrotron break frequencies in the line-of-sight integrals.

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