Titlebook: Cosmic Radiation in Contemporary Astrophysics; Maurice M. Shapiro Book 1986 D. Reidel Publishing Company, Dordrecht, Holland 1986 Populati

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Jocose

Supporting Online Credibility Evaluation,of studies of cosmic ray interactions is examined with particular reference to the information about the ISM itself which comes from observations of the flux of secondary γ-rays produced by cosmic ray interactions with gas, the situation regarding molecular gas in the Inner Galaxy being of particular concern.

稱贊

1389-2185 various astrophysical specialties, such as radio- astronomy, optical astronomy, X-ray astronomy, gamma-ray astronomy, and of course, particle astronomy (i.e., 978-94-010-8922-7978-94-009-5488-5Series ISSN 1389-2185

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Synthesis of Ideas on Cosmic Ray Origin and Propagationudo-continuous acceleration appears to require that the bulk of the particle acceleration occurs in a very large Galactic halo, the secondaries being produced only in the gas disk. Problems are likely, however, with the expected fluxes of X-rays and radio synchrotron radiation.

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Assessment by Feedback in the On-demand Era the coexistence of monoenergetic, power law, exponential and relativistic Maxwellian particle spectra. Since this variety of particle spectra is seen in cosmic sources, our results are very encouraging and definitely in favour of continuous acceleration models. Finally the secondary/primary ratio i

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A Fair Wage for Workers On-demand via Appudo-continuous acceleration appears to require that the bulk of the particle acceleration occurs in a very large Galactic halo, the secondaries being produced only in the gas disk. Problems are likely, however, with the expected fluxes of X-rays and radio synchrotron radiation.

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https://doi.org/10.1007/978-3-319-77968-3ntributors to the X-ray background and conclude that they, together with the quasars, contribute about 60 percent of the observed background. About half of this is contributed by active galactic nuclei with optical luminosities below those of quasars.