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Volumn 611, Issue 1 I, 2004, Pages 434-451

A steady, radiative-shock method for computing X-ray emission from colliding stellar winds in close, massive-star binaries

Author keywords

Binaries: general; Stars: early type; Stars: mass loss; Stars: winds, outflows; Stars: X rays

Indexed keywords


EID: 5644250965     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/422093     Document Type: Article
Times cited : (75)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.