Dynamic processes in Be star atmospheres. V. Helium line emissions from the outer atmosphere of λ Eridani

Astrophysical Journal

Volumn 481, Issue 1 PART I, 1997, Pages 467-478

  Smith, Myron A ^a   Cohen, D H ^b   Hubeny, I ^c   Plett, K ^a   Basri, G ^d   Johns Krull, C M ^d   MacFarlane, J J ^e   Hirata, R ^f  

^a Computer Sciences Corporation ^*  (United States)

^b UNIVERSITY OF WISCONSIN MADISON   (United States)

^c UNIVERSITIES SPACE RESEARCH ASSOCIATION   (United States)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e University of Kyoto ^*  (United States)

^f KYOTO UNIVERSITY   (Japan)

Author keywords

Line: formation; Line: profiles; Stars: atmospheres; Stars: emission line, Be; Stars: individual ( Eridani); Ultraviolet: stars

Indexed keywords

EID: 21744448481     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/304028     Document Type: Article

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