Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars
The University of Sydney · Laboratoire d’études spatiales et d’instrumentation en astrophysique · +29 more institutions
Indexed inarxivcrossrefpubmed
Abstract
No abstract available for this paper.
Citation impact
613
total citations
- FWCI
- 31.82
- Percentile
- 100%
- References
- 46
Citations per year
Authors
34- TRT. R. BeddingCorresponding
The University of Sydney
- BMB. Mosser
Laboratoire d’études spatiales et d’instrumentation en astrophysique, Centre National de la Recherche Scientifique, Sorbonne Université, Université de Versailles Saint-Quentin-en-Yvelines, Observatoire de Paris, Délégation Paris 7, Université Paris Cité
- DHDaniel Huber
The University of Sydney
- JMJ. Montalbán
University of Liège
- PGP. G. Beck
KU Leuven
Topics & keywords
Topics
Keywords
- Helium
- Stars
- Red giant
- Hydrogen
- Astronomy
- Physics
- Astrobiology
- Astrophysics
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