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Thermal-bremsstrahlung interpretation of cluster X-ray sources. (1973)

Kellogg, E. ; Silk, J. ; Murray, S. ; [et al.]

In: Other Sources

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Publication Date: 2019-06-27

Description: Analysis of the X-ray data for the extended sources in Coma, Perseus, and Virgo in terms of an isothermal gas-sphere model emitting thermal-bremsstrahlung radiation. It is found that the gas distribution is somewhat less centrally condensed than the galaxies, and that the gas mass is generally a small fraction of the binding mass of each cluster. In the case of the Coma cluster, approximately one-eighth of the binding mass (with an uncertainty of about 50%) may be in the form of hot gas at 100,000,000 K if H sub zero = 50 km/sec/Mpc.

Keywords: SPACE RADIATION

Type: Astrophysical Journal; 184; Sept. 15

Format: text

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