Carbon and oxygen isotopic ratios in Arcturus and Aldebaran: Constraining the parameters for non-convective mixing on the red giant branch

Astronomy and Astrophysics

Volumn 548, Issue , 2012, Pages

  Abia, C ^a   Palmerini, S ^a   Busso, M ^b   Cristallo, S ^c  

^a UNIVERSITY OF GRANADA   (Spain)

^b UNIVERSITY OF PERUGIA   (Italy)

^c INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

Author keywords

Stars: abundances; Stars: individual: Aldebaran; Stars: individual: Arcturus; Stars: late type

Indexed keywords

CARBON; CHEMICAL ELEMENTS; FORECASTING; MIXING; OXYGEN; SPECTROSCOPY;

ACE-FTS; CONVECTIVE MIXING; DIFFUSIVE PROCESS; EVOLUTIONARY MODELS; EVOLUTIONARY STAGE; FAST TRANSPORT; HIGH-RESOLUTION INFRARED SPECTRA; INITIAL COMPOSITION; ISOTOPIC ABUNDANCES; ISOTOPIC RATIOS; MOLECULAR LINES; OBSERVED DATA; OXYGEN ISOTOPIC; PARAMETRIC MODELS; PHYSICAL NATURE; RED GIANT BRANCHES; RED GIANTS; SOLAR SPECTRUM; SPECTRAL RANGE; SPECTRAL SYNTHESIS; STARS: ABUNDANCES; STARS: INDIVIDUAL: ALDEBARAN; STARS: INDIVIDUAL: ARCTURUS; STARS:LATE TYPE; STELLAR MASS; STELLAR PARAMETERS; UNCERTAIN PARAMETERS;

STARS;

EID: 84870044845     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220148     Document Type: Article

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