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Volumn 388, Issue 3, 2002, Pages 899-916

Non-radial pulsation, rotation and outburst in the Be star ω Orionis from the MuSiCoS 1998 campaign

(29)  Neiner, C a,b   Hubert, A M a   Floquet, M a   Jankov, S c,d   Henrichs, H F b   Foing, B e   Oliveira, J e,f   Orlando, S e,g   Abbott, J h,i   Baldry, I K j   Bedding, T R j   Cami, J b   Cao, H k   Catala, C l   Cheng, K P m   Domiciano De Souza Jr , A c,n   Janot Pacheco, E a,n   Hao, J X k   Kaper, L b   Kaufer, A o   more..


Author keywords

[No Author keywords available]

Indexed keywords

ALGORITHMS; CARBON; HYDROGEN; MAGNESIUM PRINTING PLATES; SIGNAL TO NOISE RATIO; SILICON; SPECTROSCOPIC ANALYSIS; TIME SERIES ANALYSIS;

EID: 0036611908     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20020522     Document Type: Article
Times cited : (36)

References (70)
  • 12
    • 0009796490 scopus 로고    scopus 로고
    • Atlas of Be stars on the web
    • (2001)
    • Buil, C.1
  • 20
    • 0009796492 scopus 로고    scopus 로고
    • Master's Thesis, IAG-USP, Brazil
    • (1997)
    • Emilio, M.1
  • 65
    • 0009751279 scopus 로고    scopus 로고
    • The be phenomenon in early-type stars
    • IAU Coll. 175, ed. M. A. Smith, H. F. Henrichs, & J. Fabregat
    • (2000) ASP Conf. Ser. , vol.214 , pp. 288
    • Townsend, R.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.