The structure of the Virgo cluster X-ray source

Details The structure of the Virgo cluster X-ray source The structure of the Virgo cluster X-ray source

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.183p..39d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 183, May 1978, p. 39P-43P.

Astronomy and Astrophysics

Astronomy

16

Galactic Clusters, Satellite Observation, Virgo Galactic Cluster, X Ray Sources, Energy Spectra, Galactic Structure, Proportional Counters, Spaceborne Astronomy, Uhuru Satellite, X Ray Stars

Scientific paper

Evidence is presented for the presence of a second extended X-ray emission region in the Virgo cluster in addition to that which is known to surround M87. This second region, which dominates at energies above about 7 keV, is located in the vicinity of M84 and 86. The presence of two distinct emission regions at different temperatures provides a natural explanation for the observation by several experimental groups of a power-law energy spectrum.

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