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Volumn 386, Issue 2, 2002, Pages 456-463
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Modeling the interaction between ICM and relativistic plasma in cooling flows: The case of the Perseus cluster
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Author keywords
Acceleration of particles; Galaxies: clusters: general; Galaxies: clusters: individual: Perseus (A426); Galaxies: cooling flows; Radiation mechanisms: non thermal
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Indexed keywords
COOLING;
ELECTRONS;
GALAXIES;
RADIO ASTRONOMY;
TURBULENCE;
X RAYS;
RADIO MINI-HALOS;
SYNCHROTRON RADIATION;
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EID: 0036569134
PISSN: 00046361
EISSN: None
Source Type: Journal
DOI: 10.1051/0004-6361:20020284 Document Type: Article |
Times cited : (160)
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References (44)
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