Fast rotating massive stars and the origin of the abundance patterns in galactic globular clusters
University of Geneva · Centre National de la Recherche Scientifique · +2 more institutions
Indexed inarxivcrossrefdoaj
Abstract
Aims.We propose the Wind of Fast Rotating Massive Stars scenario to explain the origin of the abundance anomalies observed in globular clusters.
Citation impact
710
total citations
- FWCI
- 30.15
- Percentile
- 100%
- References
- 86
Citations per year
Authors
5- TDT. DecressinCorresponding
University of Geneva
- GMG. Meynet
University of Geneva
- CCC. Charbonnel
Centre National de la Recherche Scientifique, Université Toulouse III - Paul Sabatier, University of Geneva
- NPNikos Prantzos
Institut d'Astrophysique de Paris, Centre National de la Recherche Scientifique
- SESylvia Ekström
University of Geneva
Topics & keywords
Topics
Keywords
- Globular cluster
- Stars
- Abundance (ecology)
- Physics
- Astrophysics
- Astronomy
- Star cluster
- Biology
No related works found for this paper.