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Volumn 584, Issue 1 I, 2003, Pages 418-426

Understanding the radio emission geometry of multiple-component radio pulsars from retardation and aberration effects

Author keywords

Pulsars: general; Radiation mechanisms: nonthermal; Stars: magnetic fields; Stars: neutron

Indexed keywords


EID: 0038218513     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/345682     Document Type: Article
Times cited : (91)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.