A Powerful Radio Halo in the Hottest Known Cluster of Galaxies 1E 0657−56
Author(s) -
Haida Liang,
R. W. Hunstead,
M. Birkinshaw,
P. Andreani
Publication year - 2000
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/317223
Subject(s) - radio halo , halo , physics , astrophysics , intracluster medium , cluster (spacecraft) , galaxy cluster , radio galaxy , astronomy , galaxy , computer science , programming language
We report the detection of a diffuse radio halo source in the hottest knowncluster of galaxies 1E0657-56 (RXJ0658-5557). The radio halo has a morphologysimilar to the X-ray emission from the hot intracluster medium. The presence ofa luminous radio halo in such a hot cluster is further evidence for a steepcorrelation between the radio halo power and the X-ray temperature. We favourmodels for the origin of radio halo sources involving a direct connectionbetween the X-ray emitting thermal particles and the radio emittingrelativistic particles.Comment: 21 pages of text, 9 figures, to appear in Ap
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom