The Perseus and Coma clusters of galaxies at energies above 20 keV

Details The Perseus and Coma clusters of galaxies at energies above 20 keV The Perseus and Coma clusters of galaxies at energies above 20 keV

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...205l..65s&link_type=abstract

Astrophysical Journal, vol. 205, Apr. 15, 1976, pt. 2, p. L65-L68.

Astronomy and Astrophysics

Astronomy

28

Energy Spectra, Galactic Clusters, X Ray Astronomy, X Ray Sources, Balloon-Borne Instruments, Bremsstrahlung, X Ray Spectra, X Ray Telescopes

Scientific paper

Observations of the Perseus and Coma clusters of galaxies were made on June 21, 1974, with a balloon-borne X-ray telescope (energies of approximately 20-150 keV). No positive detection was made. The data favor a thermal bremsstrahlung mechanism for the X-ray production in the Perseus cluster of galaxies over the inverse Compton mechanism. In the case of the Coma cluster of galaxies, the data are inconclusive with respect to determining the origin of the X-rays.

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