Energy spectra of X-ray clusters of galaxies

Details Energy spectra of X-ray clusters of galaxies Energy spectra of X-ray clusters of galaxies

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...210..642a&link_type=abstract

Astrophysical Journal, vol. 210, Dec. 15, 1976, pt. 1, p. 642-646. Research supported by the Israel Academy of Sciences and Hum

Astronomy and Astrophysics

Astrophysics

478

Energy Spectra, Galactic Clusters, Statistical Analysis, X Ray Sources, X Ray Spectra, Computerized Simulation, Monte Carlo Method, Range (Extremes), Spectral Energy Distribution, Spectrum Analysis

Scientific paper

A procedure for estimating the ranges of parameters that describe the spectra of X-rays from clusters of galaxies is presented. The applicability of the method is proved by statistical simulations of cluster spectra; such a proof is necessary because of the nonlinearity of the spectral functions. Implications for the spectra of the Perseus, Coma, and Virgo clusters are discussed. The procedure can be applied in more general problems of parameter estimation.

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