X ray cluster counts: What ROSAT should see

Details X ray cluster counts: What ROSAT should see X ray cluster counts: What ROSAT should see

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991tpsu.rept..127e&link_type=abstract

In MPI für Physik und Astrophysik, Traces of the Primordial Structure in the Universe p 127-142 (SEE N92-29833 20-90)

Astronomy and Astrophysics

Astronomy

1

Galactic Clusters, Galactic Structure, Red Shift, Rosat Mission, X Ray Astronomy, X Ray Sources, Astronomical Models, Dark Matter, Galactic Evolution, Luminosity

Scientific paper

Expectations for characteristics of the x-ray cluster population
observable by Rosat (x-ray astronomy satellite) are presented. The
modeling requires an initial fluctuation spectrum and relations
describing the behavior of cluster x-ray luminosity and core radius with
cluster binding mass and red shift.

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