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ASCA Observation of A1674

Published online by Cambridge University Press:  25 May 2016

T. Takai ,
K. Hayashida ,
K. Hashimotodani  and
W. Kawasaki
T. Takai
Affiliation:
Dept. of Earth & Space Science, Faculty of Science, Osaka University 1-1 Machikaneyama-cho Toyonaka-shi Osaka Japan
K. Hayashida
Affiliation:
Dept. of Earth & Space Science, Faculty of Science, Osaka University 1-1 Machikaneyama-cho Toyonaka-shi Osaka Japan
K. Hashimotodani
Affiliation:
Dept. of Earth & Space Science, Faculty of Science, Osaka University 1-1 Machikaneyama-cho Toyonaka-shi Osaka Japan
W. Kawasaki
Affiliation:
Dept. of Astronomy, School of Science, University of Tokyo 7-3-1 Hongo Bunkyo-ku Tokyo Japan

Extract

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A cluster of galaxies Abell 1674 is a nearby cluster(z=0.106) and an unique sample among Briel & Henry's(1993, A&A 278,379) catalogue. Although it has the largest number of galaxies within the Abell radius, 165, its X-ray luminosity measured in the ROSAT all-sky survey is 5 × 1043erg/s (in 0.5-2.5keV), about one order of magnitude lower than the brightest one.

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 323 - 324
Copyright
Copyright © Kluwer 1998