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Volumn 336, Issue 3, 1998, Pages 980-985

How thin B[e] supergiant disks can be?

Author keywords

Circumstellar matter; Stars: Emission line, be; Stars: Mass loss; Stars: Supergiants

Indexed keywords


EID: 2142660756     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (3)

References (15)
  • 8
    • 11644306027 scopus 로고    scopus 로고
    • Paris, Hubert, A-M. & Jaschek, M. eds, Kluwer Academic Publishers, in press
    • Pacheco, J.A. 1998, Workshop on B[e] stars, Paris, Hubert, A-M. & Jaschek, M. eds, Kluwer Academic Publishers, in press
    • (1998) Workshop on B[e] Stars
    • Pacheco, J.A.1
  • 13
    • 0008575066 scopus 로고
    • Davidson K., Moffat A.F.J., Lamers H.J.G.L.M., eds, Kluwer Academic Publishers, Dordrecht
    • Zickgraf F.-J. 1990, in Davidson K., Moffat A.F.J., Lamers H.J.G.L.M., eds, IAU Colloquium 113, Kluwer Academic Publishers, Dordrecht, p. 117
    • (1990) IAU Colloquium , vol.113 , pp. 117
    • Zickgraf, F.-J.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.