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Volumn 556, Issue , 2013, Pages

A representative sample of Be stars: V. H α variability

Author keywords

Circumstellar matter; Stars: emission line, Be

Indexed keywords

CIRCUMSTELLAR MATTERS; DEGREE OF VARIABILITY; LINE STRENGTH; LUMINOSITY CLASS; PHASE CHANGE; REPRESENTATIVE SAMPLE; SPECTRAL TYPES; STARS: EMISSION-LINE , BE;

EID: 84881089493     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220419     Document Type: Article
Times cited : (29)

References (27)
  • 4
    • 65249136152 scopus 로고
    • eds. A. Slettebak, & T. P. Snow, IAU Colloq
    • Collins, II, G. W. 1987, in Physics of Be Stars, eds. A. Slettebak, & T. P. Snow, IAU Colloq., 92, 3
    • (1987) Physics of Be Stars , vol.92 , pp. 3
    • Collins, I.I.G.W.1
  • 10
    • 0042804790 scopus 로고
    • eds. M. Jaschek, & H.-G. Groth, IAU Symp
    • Jaschek, M., & Egret, D. 1982, in Be Stars, eds. M. Jaschek, & H.-G. Groth, IAU Symp., 98, 261
    • (1982) Be Stars , vol.98 , pp. 261
    • Jaschek, M.1    Egret, D.2
  • 12
    • 0040508616 scopus 로고
    • Kogure, T. 1990, Ap&SS, 163, 7
    • (1990) Ap&SS , vol.163 , pp. 7
    • Kogure, T.1
  • 13


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.