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Volumn 386, Issue 2, 2002, Pages 456-463

Modeling the interaction between ICM and relativistic plasma in cooling flows: The case of the Perseus cluster

Author keywords

Acceleration of particles; Galaxies: clusters: general; Galaxies: clusters: individual: Perseus (A426); Galaxies: cooling flows; Radiation mechanisms: non thermal

Indexed keywords

COOLING; ELECTRONS; GALAXIES; RADIO ASTRONOMY; TURBULENCE; X RAYS;

EID: 0036569134     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20020284     Document Type: Article
Times cited : (160)

References (44)


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.