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Astrophysical Journal

Volumn 764, Issue 1, 2013, Pages

Theoretical explanation of the cosmic-ray perpendicular diffusion coefficient in the nearby starburst galaxy NGC 253

(3) Buffie, K a Heesen, V b Shalchi, A a

a UNIVERSITY OF MANITOBA (Canada)

b UNIVERSITY OF SOUTHAMPTON (United Kingdom)

Author keywords

cosmic rays; galaxies: individual (NGC 253); galaxies: magnetic fields; galaxies: starburst

Indexed keywords

EID: 84873973414 PISSN: 0004637X EISSN: 15384357 Source Type: Journal
DOI: 10.1088/0004-637X/764/1/37 Document Type: Article

Times cited : (23)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.