The nine lives of cosmic rays in galaxies
Reviewartikel, 2015

Cosmic-ray astrophysics has advanced rapidly in recent years, and its impact on other astronomical disciplines has broadened. Many new experiments measuring these particles, both directly in the atmosphere or space and indirectly via γ rays and synchrotron radiation, have widened the range and quality of the information available on their origin, propagation, and interactions. The impact of low-energy cosmic rays on interstellar chemistry is a fast-developing topic, including the propagation of these particles into the clouds in which the chemistry occurs. Cosmic rays, via their γ-ray production, also provide a powerful way to probe the gas content of the interstellar medium. Substantial advances have been made in the observations and modelling of the interplay between cosmic rays and the interstellar medium. Focusing on energies up to 1 TeV, these interrelating aspects are covered at various levels of detail, giving a guide to the state of the subject.

Dust

γ rays

Interstellar medium

Superbubbles

Interstellar chemistry

Författare

I.A. Grenier

Centre national de la recherche scientifique (CNRS)

John H Black

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

A.W. Strong

Max-Planck-Gesellschaft

Annual Review of Astronomy and Astrophysics

0066-4146 (ISSN) 1545-4282 (eISSN)

Vol. 53 1 199-246

Ämneskategorier

Subatomär fysik

Astronomi, astrofysik och kosmologi

Fundament

Grundläggande vetenskaper

Infrastruktur

Onsala rymdobservatorium

DOI

10.1146/annurev-astro-082214-122457

Mer information

Senast uppdaterat

2021-07-12