The DOI matches its Crossref record; 25 of the 25 references it cites were found in a registry or an index.
Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars
Open accessAbstract
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 by 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 ∼50 seconds) and those that are also burning helium (period spacing ∼100 to 300 seconds).
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Cites
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Asymptotic approximations for stellar nonradial pulsations
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Correcting Stellar Oscillation Frequencies for Near-Surface Effects
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Self-citationINITIAL CHARACTERISTICS OF KEPLER LONG CADENCE DATA FOR DETECTING TRANSITING PLANETS
Jenkins, J. M., Caldwell, D. A., Chandrasekaran, H., Twicken, J. D., Bryson, S. T., Quintana, E. V., Clarke, B. D., Li, J., Allen, C., Tenenbaum, P., et al. (2010) · The Astrophysical Journal · doi:10.1088/2041-8205/713/2/l120 · Cited by 333
Self-citationNon-radial oscillation modes with long lifetimes in giant stars
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Self-citationASTEC—the Aarhus STellar Evolution Code
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Self-citationSOLAR-LIKE OSCILLATIONS IN LOW-LUMINOSITY RED GIANTS: FIRST RESULTS FROM KEPLER
Bedding, T. R., Huber, D., Stello, D., Elsworth, Y. P., Hekker, S., Kallinger, T., Mathur, S., Mosser, B., Preston, H. L., Ballot, J., et al. (2010) · The Astrophysical Journal · doi:10.1088/2041-8205/713/2/l176 · Cited by 240
Self-citationKepler Detected Gravity-Mode Period Spacings in a Red Giant Star
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Self-citationTheoretical amplitudes and lifetimes of non-radial solar-like oscillations in red giants
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Self-citationAmplitudes of Stellar Oscillations: The Implications for AsteroseismologyPreprint
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Cited by
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Self-citationStellar Spin-Orbit Misalignment in a Multiplanet System
Huber, D., Carter, J. A., Barbieri, M., Miglio, A., Deck, K. M., Fabrycky, D. C., Montet, B. T., Buchhave, L. A., Chaplin, W. J., Hekker, S., et al. (2013) · Science · doi:10.1126/science.1242066 · Cited by 315
Self-citationPLANETARY CANDIDATES OBSERVED BY KEPLER . VI. PLANET SAMPLE FROM Q1–Q16 (47 MONTHS)
Mullally, F., Coughlin, J. L., Thompson, S. E., Rowe, J., Burke, C., Latham, D. W., Batalha, N. M., Bryson, S. T., Christiansen, J., Henze, C. E., et al. (2015) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/217/2/31 · Cited by 254
Self-citationGirardi, L. (2016) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081915-023354 · Cited by 242
Metadata
- Authors
- Bedding, T. R., Mosser, B., Huber, D., Montalbán, J., Beck, P., Christensen-Dalsgaard, J., Elsworth, Y. P., García, R. A., Miglio, A., Stello, D., White, T. R., De Ridder, J., Hekker, S., Aerts, C., Barban, C., Belkacem, K., Broomhall, A.-M., Brown, T. M., Buzasi, D. L., Carrier, F., Chaplin, W. J., Di Mauro, M. P., Dupret, M.-A., Frandsen, S., Gilliland, R. L., Goupil, M.-J., Jenkins, J. M., Kallinger, T., Kawaler, S., Kjeldsen, H., Mathur, S., Noels, A., Aguirre, V. S., & Ventura, P.
- Venue
- Nature
- Published
- 2011-03
- Volume
- 471
- Issue
- 7340
- Pages
- 608-611
- ISSN
- 0028-0836 (ISSN-L)
- 1476-4687
- OpenAlex
- W2108910145
- Cited by
- 608
- References
- 25
- FWCI
- 26.27
- Type
- journal article
- Language
- en
- Open access
- bronze
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- The paper
- Bedding, T. R., Mosser, B., Huber, D., Montalbán, J., Beck, P., Christensen-Dalsgaard, J., Elsworth, Y. P., García, R. A., Miglio, A., Stello, D., White, T. R., De Ridder, J., Hekker, S., Aerts, C., Barban, C., Belkacem, K., Broomhall, A.-M., Brown, T. M., Buzasi, D. L., . . . Ventura, P. (2011). Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars. Nature. https://doi.org/10.1038/nature09935
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