SUMMARY OF PROPOSAL 71151
UNIVERSITY OF TOKYO
7-3-1 HONGO
BUNKYO-KU
TOKYO JAPAN 113
Tel: 03-3812-2111 EXT. 4204 Fax: 03-3815-8875
Medium: CD-ROM
Subject: CLUSTERS OF GALAXIES AND SUPERCLUSTERS
OBSERVATION OF THE SHOCK FRONTS ALONG THE RIM OF A3667 CLUSTER.
ABSTRACT
Among several known cluster radio haloes, we found one good candidate for the site of ultra-high-energy cosmic rays, a pair of shock fronts along the rim of A3667. They have outstanding characteristics as a cosmic accelerator: located at the rim where massive accretion is taking place, extending about 1 Mpc, their power index of radio emission very close to 1. We expect to find the first direct proof of the acceleration up to 10^20 eV in the cluster scale structure with ASCA.
CO-INVESTIGATORS
CO-I NAME | INSTITUTE | COUNTRY |
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MOTOHIDE KOKUBUN | UNIVERSITY OF TOKYO | JAPAN |
YASUSHI FUKAZAWA | UNIVERSITY OF TOKYO | JAPAN |
KEIICHI MATSUZAKI | UNIVERSITY OF TOKYO | JAPAN |
TAKASHI OHSUGI | HIROSHIMA UNIVERSITY | JAPAN |
TARGETS
TARGET NAME | PRI | RA | DEC | TIME | TC | OFF | GIS | SIS CNT | OBS |
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1)A3667 2006-56 | A | 302.5000 | -56.4167 | 50 ks | N | Y | P | 0.01000 | 1 |
2)A3667 2010-57 | A | 303.5000 | -57.0000 | 50 ks | N | Y | P | 0.01000 | 1 |