Cosmic rays from the Galactic center - Path length distributions and Galactic gradient in a modified model

Details Cosmic rays from the Galactic center - Path length distributions and Galactic gradient in a modified model Cosmic rays from the Galactic center - Path length distributions and Galactic gradient in a modified model

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...390..105w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 390, no. 1, May 1, 1992, p. 105-107.

Astronomy and Astrophysics

Astrophysics

1

Cosmic Rays, Galactic Nuclei, Milky Way Galaxy, Astronomical Models, Halos, Particle Flux Density

Scientific paper

The paper presents a number of modifications of the Galactic center
production model for cosmic rays (CRs). They allow the reproduction of
data on the CR Galactic gradient as well as the secondary to primary
ratios. The energy dependence of these characteristics is found to be in
general agreement with the data.

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