Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars
arXiv:1103.5805 · doi:10.1038/nature09935
Abstract
Red giants are evolved stars that have exhausted the supply of hydrogen in their cores and instead burn hydrogen in a surrounding shell. Once a red giant is sufficiently evolved, the helium in the core also undergoes fusion. Outstanding issues in our understanding of red giants include uncertainties in the amount of mass lost at the surface before helium ignition and the amount of internal mixing from rotation and other processes. Progress is hampered by our inability to distinguish between red giants burning helium in the core and those still only burning hydrogen in a shell. Asteroseismology offers a way forward, being a powerful tool for probing the internal structures of stars using their natural oscillation frequencies. Here we report observations of gravity-mode period spacings in red giants that permit a distinction between evolutionary stages to be made. We use high-precision photometry obtained with the Kepler spacecraft over more than a year to measure oscillations in several hundred red giants. We find many stars whose dipole modes show sequences with approximately regular period spacings. These stars fall into two clear groups, allowing us to distinguish unambiguously between hydrogen-shell-burning stars (period spacing mostly about 50 seconds) and those that are also burning helium (period spacing about 100 to 300 seconds).
to appear as a Letter to Nature
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- Is there a unique asteroseismic interior model for the solar-like oscillating KIC 7747078?
- Stellar oscillations - the adiabatic case
- Chronos --- Taking the pulse of our Galactic neighbourhood (ESA Voyage 2050 White Paper)
- Concerning Li-rich status of KIC~9821622: A Kepler field RGB star reported as Li-rich Giant
- Constraining stellar physics from red-giant stars in binaries - stellar rotation, mixing processes and stellar activity
- Fundamental stellar properties from asteroseismology
- Seismic and spectroscopic analysis of 9 bright red giants observed by Kepler
- Red giant asteroseismic binaries in the Kepler field
- The AGB bump: a calibrator for the core mixing
- Contributions of structural variations to the asymptotic mixed-mode coupling Factor in red giant stars
- Seismic indices -- a deep look inside evolved stars
- Asteroseismology
- The γ Dor stars as revealed by Kepler : A key to reveal deep-layer rotation in A and F stars
- Asteroseismology of red giants & galactic archaeology
- The Tale of a Hungry Subgiant and Its Brown Dwarf: Interior Radiative Damping Dominates the Tidal Evolution of TOI-5882
- Early Results from APOKASC
- Calibration of the [C/N] and [Y/Mg] chemical clocks with asteroseismic ages from the TESS space mission
- Asymptotic power spectra and visibilities of damped mixed modes
- Spectroscopic and asteroseismic analysis of the secondary clump red giant HD 226808
- The noise wars in helio- and asteroseismology
- Detailed theoretical analysis of core Helium-burning stars: Mixed mode patterns I. Impact of the He-flash discontinuity and of induced semi-convection
- HAYDN -- High-precision AsteroseismologY of DeNse stellar fields (ESA Voyage 2050 White Paper)
- Asteroseismic Analysis of a Red Giant KIC 9145955 by Including the Small-scale Magnetic Fields in the Atmosphere
- Physical interpretation of the oscillation spectrum on the RGB and AGB
- Kepler Pixel Project -- background RR Lyrae stars in the primary Kepler mission field of view
- Probing the Deep End of the Milky Way with New Oscillating Kepler Giants
- Asteroseismology of iota Draconis and Discovery of an Additional Long-Period Companion
- Hidden oscillations in plain sight: identification of seismically unresolved red-giant asteroseismic binary candidates
- New population synthesis approach:The golden path to constrain stellar andgalactic physics
- Isochrone-cloud fitting and asteroseismology of the Kepler open cluster NGC6866
- Peak Bagging of red giant stars observed by Kepler: first results with a new method based on Bayesian nested sampling
- A Near-Infrared and Optical Study of NGC 5822: An Open Cluster Hosting Barium-stars and Lithium-Enriched Giant Stars
- Perspectives on the Physics of Late-Type Stars from Beyond Low Earth Orbit, the Moon and Mars
- Precision Analysis of Evolved Stars
- Stellar activity cycles and contribution of the deep layers knowledge