V453 Oph: A s-process enriched, but carbon-deficient RV Tauri star of low intrinsic metallicity

Astronomy and Astrophysics

Volumn 438, Issue 3, 2005, Pages 987-998

  Deroo, P ^a   Reyniers, M ^a   Van Winckel, H ^a   Goriely, S ^b   Siess, L ^b  

^a KU LEUVEN   (Belgium)

^b UNIVERSITÉ LIBRE DE BRUXELLES   (Belgium)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: AGB and post AGB; Stars: evolution; Stars: individual: DS Aqr; Stars: individual: V453 Oph

Indexed keywords

CARBON; CONDENSATION; MATHEMATICAL MODELS; MONITORING; NEUTRONS; NITROGEN; OPTICAL RESOLVING POWER; PHOTOMETRY; SIGNAL TO NOISE RATIO; SPECTROGRAPHS; SPECTROSCOPIC ANALYSIS; THERMAL EFFECTS;

NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES; STARS: ABUNDANCES; STARS: AGB AND POST-AGB; STARS: EVOLUTION; STARS: INDIVIDUAL: DS AQR; STARS: INDIVIDUAL: V453 OPH;

ASTROPHYSICS;

EID: 23744489844     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041858     Document Type: Article

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