The natural pulse of a red-giant star provides crucial insight into what makes it shine. Observations of red giants by the Kepler space telescope shed light on a previously untested prediction of stellar evolution theory. See Letter p.608
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on SpringerLink
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
References
Bedding, T. R. et al. Nature 471, 608–611 (2011).
Silvotti, R. et al. Nature 449, 189–191 (2007).
Aerts, C., Christensen-Dalsgaard, J., Cunha, M. & Kurtz, D. W. Sol. Phys. 251, 3–20 (2008).
Borucki, W. J. et al. Astrophys. J. 728, 117–137 (2011).
Gilliland, R. et al. Publ. Astron. Soc. Pacif. 122, 131–143 (2010).
Chaplin, W. J. et al. Science (in the press).
Beck, P. G. et al. Science doi:10.1126/science.1201939 (2011).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Metcalfe, T. The inner lives of red giants. Nature 471, 580–581 (2011). https://doi.org/10.1038/471580a
Published:
Issue Date:
DOI: https://doi.org/10.1038/471580a