The X-ray spectra of cluster cooling flows. I - Optically thin models

Details The X-ray spectra of cluster cooling flows. I - Optically thin models The X-ray spectra of cluster cooling flows. I - Optically thin models

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...415...58w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 415, no. 1, p. 58-74.

Astronomy and Astrophysics

Astrophysics

15

Cooling Flows (Astrophysics), Galactic Clusters, X Ray Spectra, Astronomical Models, X Ray Astronomy

Scientific paper

Calculations are carried out of optically thin X-ray spectra for a set of theoretical cluster cooling flow models including homogeneous models and flows with strong gas loss. Integrated X-ray properties for the models are presented, together with surface brightness profiles, aperture luminosities, and line profiles for a representative set of X-ray lines. It is found that models with gas loss have lower total X-ray luminosities than homogeneous models by a factor of 1.35 or less.

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