The mercury-manganese binary star φ Herculis: Detection and properties of the secondary and revision of the elemental abundances of the primary

Astrophysical Journal

Volumn 655, Issue 2 I, 2007, Pages 1046-1057

  Zavala, R T ^a   Adelman, S J ^b,c   Hummel, C A ^d   Gulliver, A F ^c,e   Caliskan, H ^f   Armstrong, J T ^g   Hutter, D J ^a   Johnston, K J ^h   Pauls, T A ^g  

^a FLAGSTAFF STATION   (United States)

^b THE CITADEL   (United States)

^c NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^d EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^e BRANDON UNIVERSITY   (Canada)

^f ISTANBUL UNIVERSITY   (Turkey)

^g NAVAL RESEARCH LABORATORY   (United States)

^h US NAVAL OBSERVATORY   (United States)

Author keywords

Astrometry; Binaries: spectroscopic; Stars: abundances; Stars: chemically peculiar; Stars: individual ( Herculis AB)

Indexed keywords

EID: 33847207752     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/510108     Document Type: Article

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