The Effects of Rotation on Cooling Flows

Details The Effects of Rotation on Cooling Flows The Effects of Rotation on Cooling Flows

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...185.5302g&link_type=abstract

American Astronomical Society, 185th AAS Meeting, #53.02; Bulletin of the American Astronomical Society, Vol. 26, p.1402

Astronomy and Astrophysics

Astronomy

Scientific paper

Recent observations suggest that rotation may be dynamically significant in the cores of some cooling flow clusters (e.g. Hydra-A). We have therefore begun to investigate the effect of rotation on the properties of cooling flows. This was performed by first computing a spherically symmetric cooling flow in the gravitational potential of an elliptical galaxy and King model cluster distribution. The 1D solution was perturbed by applying a rotation and its evolution followed using an axisymmetric hydrodynamical code. The effects of different rotation profiles and rotation strengths have been studied, and will be presented.

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