On the low energy X-ray absorption of the Coma, Virgo and Perseus Clusters

Details On the low energy X-ray absorption of the Coma, Virgo and Perseus Clusters On the low energy X-ray absorption of the Coma, Virgo and Perseus Clusters

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....68..281b&link_type=abstract

Astronomy and Astrophysics, vol. 68, no. 1-2, Aug. 1978, p. 281-287.

Astronomy and Astrophysics

Astrophysics

3

Galactic Clusters, Stellar Spectra, Virgo Galactic Cluster, X Ray Sources, Ariel 5 Satellite, Astronomical Netherlands Satellite, Bremsstrahlung, Compton Effect, Photon Density, Thermal Radiation

Scientific paper

X-ray data from the soft and medium energy X-ray experiments (0.15-8 keV) on board ANS for the Coma, Perseus and Virgo Clusters are presented. The derived spectral parameters above 2 keV are in general agreement with the Uhuru, Ariel V and OSO-8 data. Due to the availability of a low-energy channel around 0.25 keV, further limits on the low energy absorption have been determined.

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