Elemental abundance analyses with DAO spectrograms - XIV. The double-lined spectroscopic binary 112 Herculis

Monthly Notices of the Royal Astronomical Society

Volumn 283, Issue 4, 1996, Pages 1115-1132

  Ryabchikova, T A ^a   Zakharova, L A ^a   Adelman, S J ^b,c  

^a INSTITUTE OF ASTRONOMY   (Russian Federation)

^b THE CITADEL   (United States)

^c NATIONAL RESEARCH COUNCIL CANADA   (Canada)

Author keywords

Binaries: spectroscopic; Stars: abundances; Stars: chemically peculiar; Stars: individual: 112 Her

Indexed keywords

BINARY ALLOYS; MANGANESE; MERCURY AMALGAMS; STARS;

ABUNDANCE ANALYSIS; BINARIES: SPECTROSCOPIC; ELEMENTAL ABUNDANCE; HIGH RESOLUTION; SPECTROGRAMS; SPECTROSCOPIC BINARY; STAR: INDIVIDUAL: 112 HER; STARS ABUNDANCES; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: PROXIMA CENTAURI;

MANGANESE ALLOYS;

EID: 0000570078     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/283.4.1115     Document Type: Article

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