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X-Ray Properties of ASCA Observed 43 Clusters of Galaxies

Published online by Cambridge University Press:  25 May 2016

F. Akimoto ,
M. Watanabe ,
A. Furuzawa ,
Y. Tawara ,
Y. Kumai ,
S. Satoh  and
K. Yamashita
F. Akimoto
Affiliation:
Department of Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-01, Japan [email protected]
M. Watanabe
Affiliation:
Department of Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-01, Japan [email protected]
A. Furuzawa
Affiliation:
Department of Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-01, Japan [email protected]
Y. Tawara
Affiliation:
Department of Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-01, Japan [email protected]
Y. Kumai
Affiliation:
Department of Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-01, Japan [email protected]
S. Satoh
Affiliation:
Department of Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-01, Japan [email protected]
K. Yamashita
Affiliation:
Department of Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-01, Japan [email protected]

Extract

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Much attempts of statistical approach have been made to study the origin of heavy elements, distribution of dark matter and evolution of clusters of galaxies. Henry et al.(1991) reported a power-law relation; LX ∝ kTγ, γ ~ 2.7. Edge and Stwert(1991) found significant scatter in the correlation using 45 clusters. David at al.(1993) reported γ ~ 3.4 using 104 clusters.

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 295 - 296
Copyright
Copyright © Kluwer 1998 

References

Edge, and Stwert, 1991, MNRAS, 252, 414 CrossRefGoogle Scholar
David, L. et al. 1993, ApJ, 412, 479 CrossRefGoogle Scholar
Henry, J. et al. 1991, ApJ, 372, 410 CrossRefGoogle Scholar
Scharf, and Mushotzky, 1997, ApJL Google Scholar