Halo of NGC 4631 and models of cosmic-ray transport

Details Halo of NGC 4631 and models of cosmic-ray transport Halo of NGC 4631 and models of cosmic-ray transport

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..370c&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 370-373 (SEE N85-34006 22-93)

Physics

Cosmic Rays, Energy Spectra, Halos, Models, Radiation Transport, Spiral Galaxies, Diffusion, Electrons, Height, Interstellar Matter, Magnetic Fields, Protons, Radiation Spectra

Scientific paper

The halo of edge-on spiral galaxy of NGC 4631 is studied from 327 MHz to
10700 MHz to delineate the models of cosmic-ray transport. Preliminary
studies show that the spectral steepening as a function of height above
the plane can be understood in terms of the simplest cosmic-ray
transport models, viz. simple isotropic diffusion in an infinite medium.

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