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Volumn 463, Issue 3, 2007, Pages 1111-1123

A new paradigm for the X-ray emission of O stars from XMM-Newton observations of the O9.7 supergiant ζ Orionis

Author keywords

Shock waves; Stars: early type; Stars: individual : Orionis; Stars: winds, outflows; X rays: stars

Indexed keywords

CHARGE TRANSFER; ELECTRONS; IONIZATION; LIGHT EMISSION; MAGNETIC FIELDS; SHOCK WAVES; SPECTRUM ANALYSIS; VELOCITY MEASUREMENT; WIND EFFECTS; X RAYS;

EID: 33847748577     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20053838     Document Type: Article
Times cited : (45)

References (51)
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    • Ph.D. Thesis, University of Wisconsin
    • Miller, N. A. 2002, Ph.D. Thesis, University of Wisconsin.
    • (2002)
    • Miller, N.A.1
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.