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Reaction rate uncertainties and the operation of the NeNa and MgAl chains during HBB in intermediate-mass AGB stars

Author
IZZARD, R. G1 ; LUGARO, M1 ; KARAKAS, A. I2 ; ILIADIS, C3 4 ; VAN RAAI, M1
[1] Sterrekundig Instituut, University of Utrecht, Postbus 80000 3508 TA Utrecht, Netherlands
[2] Origins Institute, Department of Physics & Astronomy, McMaster University, Hamilton ON, Canada
[3] Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599-3255, United States
[4] Triangle Universities Nuclear Laboratory, PO Box 90308, Durham, NC 27708-0308, United States
Source

Astronomy and astrophysics (Berlin. Print). 2007, Vol 466, Num 2, pp 641-648, 8 p ; ref : 1/4 p

CODEN
AAEJAF
ISSN
0004-6361
Scientific domain
Astronomy earth cosmic environment
Publisher
EDP Sciences, Les Ulis
Publication country
France
Document type
Article
Language
English
Author keyword
nuclear reactions, nucleosynthesis, abundances stars: AGB and post-AGB
Keyword (fr)
Abondance Algorithme Amas globulaire Amas stellaire Anomalie Branche géante asymptotique Effet proton Evolution chimique Evolution galactique Incertitude Masse stellaire Modèle chimique Modèle stellaire Métallicité Nucléosynthèse Réaction proton Taux capture Vitesse réaction Voie lactée
Keyword (en)
Abundance Algorithms Globular clusters Star clusters Anomaly Asymptotic giant branch Proton effects Chemical evolution Galactic evolution Uncertainty Stellar mass Chemical model Star models Metallicity Nucleosynthesis Proton reactions Capture rate Reaction rates Milky Way
Keyword (es)
Anomalía Rama gigante asintótica Evolución química Incertidumbre Modelo químico Metalicidad Tasa captura
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18696128

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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