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Volumn 375, Issue 2, 2007, Pages 657-664

The growth of baryonic structure in the presence of cosmological magnetic pressure

Author keywords

Galaxies: clusters: general; Hydrodynamics; Magnetic fields; Methods: numerical

Indexed keywords

DENSITY OF GASES; NUMERICAL METHODS;

EID: 33847003362     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.11323.x     Document Type: Article
Times cited : (6)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.