Discovery of a Large-scale Abundance Gradient in the Cluster of Galaxies AWM 7 with ASCA

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Published 1997 October 22 © 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation H. Ezawa et al 1997 ApJ 490 L33 DOI 10.1086/311004

1538-4357/490/1/L33

Abstract

A large-scale gradient in the metal abundance has been detected with ASCA from an X-ray bright cluster of galaxies, AWM 7. The metal abundance shows a peak of 0.5 solar at the center and smoothly declines to ≲0.2 solar at a radius of 500 kpc. The gas temperature is found to be constant at 3.8 keV. The radial distribution of iron can be fitted with a β model with β ~ 0.8 assuming the same core radius (115 kpc) as that of the intracluster medium. The metal distribution in AWM 7 suggests that the gas injected from galaxies is not efficiently mixed in the cluster space and traces the distribution of galaxies.

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10.1086/311004