Further studies of X-ray structure of the Perseus cluster

Details Further studies of X-ray structure of the Perseus cluster Further studies of X-ray structure of the Perseus cluster

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..230l&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 230-233 (SEE N85-33902 22-93)

Computer Science

1

Galactic Clusters, Gamma Rays, Infrared Radiation, Relativistic Electron Beams, X Ray Sources, X Rays, Atmospheric Models, Bremsstrahlung, Compton Effect

Scientific paper

The X-ray sources in the Perseus cluster have been studied by many authors. In the present study, the authors have examined and summarized available data on the spatial and spectral distributions. Based on these observations, a consistent model is proposed for the production of X-rays and γ-rays in the region around NGC 1275. It is shown that good agreement with observations is obtained by assuming the emission of soft X-rays from thermal bremsstrahlung and of hard X-rays and γ-rays from the inverse Compton process.

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