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Chandra observations of isolated early-type galaxies

Published online by Cambridge University Press:  06 October 2005

Z. Y. Huo ,
X. Y. Xia ,
S. Mao ,
S. J. Xue  and
Z. G. Deng
Z. Y. Huo
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, A20 Datun Road, 100012 Beijing, China; Email: hzy@bao.ac.cn
X. Y. Xia
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, A20 Datun Road, 100012 Beijing, China; Email: hzy@bao.ac.cn Dept. of Physics, Tianjin Normal University, 300074 Tianjin, China
S. Mao
Affiliation:
Univ. of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, UK
S. J. Xue
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, A20 Datun Road, 100012 Beijing, China; Email: hzy@bao.ac.cn
Z. G. Deng
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, A20 Datun Road, 100012 Beijing, China; Email: hzy@bao.ac.cn Dept. of Physics, Graduate School, Chinese Academy of Sciences, 100039 Beijing, China
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Abstract

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In this paper, we present a statistical study of the X-ray properties of 11 isolated early-type galaxies (IEGs) observed with the Chandra ACIS-S3, and then discuss the implications of these properties.