The evolution of cluster X-ray sources - Subcluster collisions

Details The evolution of cluster X-ray sources - Subcluster collisions The evolution of cluster X-ray sources - Subcluster collisions

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.187..371g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 187, May 1979, p. 371-378.

Astronomy and Astrophysics

Astronomy

15

Astronomical Models, Galactic Clusters, Intergalactic Media, Computerized Simulation, Luminous Intensity, X Ray Astronomy

Scientific paper

The evolution of cluster X-ray sources is investigated with a three-dimensional hydrodynamical numerical technique. Particular attention is paid to the behavior of intracluster gas during the merger of two subclusters to form a single cluster. Only a small enhancement in X-ray luminosity during the merger is found. The evolution of the X-ray luminosity subsequent to the merger is very similar to that found previously with a one-dimensional code.

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