Elemental abundance analyses with DAO spectrograms - XV. The superficially normal late B-type and early A-type stars Merak, π Draconis and κ Cephei

Monthly Notices of the Royal Astronomical Society

Volumn 280, Issue 1, 1996, Pages 130-142

  Adelman, Saul J ^a,b  

^a School of Business   (United States)

^b NATIONAL RESEARCH COUNCIL CANADA   (Canada)

Author keywords

Stars: abundances; Stars: individual: Merak; Stars: individual: Cephei; Stars: individual: Draconis

Indexed keywords

SPECTROGRAPHS;

ABUNDANCE ANALYSIS; ELEMENTAL ABUNDANCE; SPECTROGRAMS; STAR: INDIVIDUAL: MERAK; STAR: INDIVIDUAL: Κ CEPHEI; STAR: INDIVIDUAL: Π DRACONIS; STARS ABUNDANCES; STARS: INDIVIDUAL: PROXIMA CENTAURI;

STARS;

EID: 0039066804     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/280.1.130     Document Type: Article

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