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Volumn 683, Issue 2, 2008, Pages 1052-1062

The effects of clumps in explaining X-ray emission lines from hot stars

Author keywords

Line: formation; Shock waves; Stars: early type; Stars: winds, outflows; X rays: general; X rays: stars

Indexed keywords


EID: 51349140109     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/589760     Document Type: Article
Times cited : (25)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.