Elemental abundance analyses with DAO spectrograms - XVI. The normal F main-sequence stars σ Bootis, θ Cygni and τ Piscum, and the Am stars 15 Vulpeculae and 32 Aquarii

Monthly Notices of the Royal Astronomical Society

Volumn 288, Issue 2, 1997, Pages 470-500

  Adelman, Saul J ^a,c   Caliskan, Hulya ^b   Kocer, Dursun ^b   Bolcal, Cetin ^b  

^a THE CITADEL   (United States)

^b ISTANBUL UNIVERSITY   (Turkey)

^c NATIONAL RESEARCH COUNCIL CANADA   (Canada)

Author keywords

Stars: abundances; Stars: individual: 15 Vul; Stars: individual: 32 Aqr; Stars: individual: Cyg; Stars: individual: Boo; Stars: individual: Psc

Indexed keywords

RARE EARTHS;

STAR: INDIVIDUAL: 15 VUL; STAR: INDIVIDUAL: 32 AQR; STAR: INDIVIDUAL: Θ CYG; STAR: INDIVIDUAL: Σ BOO; STAR: INDIVIDUAL: Τ PSC; STARS ABUNDANCES; STARS: INDIVIDUAL: PROXIMA CENTAURI;

STARS;

EID: 0000582392     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/288.2.470     Document Type: Article

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