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Volumn 545, Issue , 2012, Pages

O Puppis: Another Be+sdO binary?

Author keywords

Binaries: close; Binaries: spectroscopic; Stars: emission line Be; Stars: individual:o Puppis

Indexed keywords

BE STARS; BINARIES: CLOSE; BINARIES: SPECTROSCOPIC; EMISSION PEAKS; HELIUM LINES; RADIAL VELOCITY CURVES; STARS: EMISSION LINES; STARS: INDIVIDUAL;

EID: 84866527469     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219679     Document Type: Article
Times cited : (58)

References (34)
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    • eds. M. A. Smith, H. F. Henrichs, & J. Fabregat, IAU Coll., 175
    • Gies, D. R. 2000, in The Be Phenomenon in Early-Type Stars, eds. M. A. Smith, H. F. Henrichs, & J. Fabregat, IAU Coll., 175
    • (2000) The Be Phenomenon in Early-Type Stars
    • Gies, D.R.1
  • 14
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    • 0000110404 scopus 로고    scopus 로고
    • Okazaki, A. T. 1997, A&A, 318, 548
    • (1997) A&A , vol.318 , pp. 548
    • Okazaki, A.T.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.