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Sodium content as a predictor of the advanced evolution of globular cluster stars
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The asymptotic giant branch (AGB) phase is the final stage of nuclear burning for low-mass stars. Although Milky Way globular clusters are now known to harbour (at least) two generations of stars, they still provide relatively homogeneous samples of stars that are used to constrain stellar evolution theory. It is predicted by stellar models that the majority of cluster stars with masses around the current turn-off mass (that is, the mass of the stars that are currently leaving the main sequence phase) will evolve through the AGB phase. Here we report that all of the second-generation stars in the globular cluster NGC 6752--70 per cent of the cluster population--fail to reach the AGB phase. Through spectroscopic abundance measurements, we found that every AGB star in our sample has a low sodium abundance, indicating that they are exclusively first-generation stars. This implies that many clusters cannot reliably be used for star counts to test stellar evolution timescales if the AGB population is included. We have no clear explanation for this observation.
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Star counts as a proxy for timescales suggest that the data argue against the reality of the breathing pulses.
“Nevertheless, appealing again to star counts as a proxy for timescales, the data seem to argue against the reality of these pulses (Renzini & Fusi Pecci 1988; Caputo et al. 1989, but see also Campbell et al. 2013).”
From The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars (2014) · cites this paper as Campbell et al. 2013
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Campbell, S. W., MacLean, B. T., D’Orazi, V., Casagrande, L., de Silva, G. M., Yong, D., Cottrell, P. L., & Lattanzio, J. C. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201731101 · Cited by 14
Self-citationOn the AGB stars of M 4: a robust disagreement between spectroscopic observations and theory
MacLean, B. T., Campbell, S. W., Amarsi, A. M., Nordlander, T., Cottrell, P. L., Silva, G. M. D., Lattanzio, J. C., Constantino, T. N., D’Orazi, V., & Casagrande, L. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2297 · Cited by 13
Self-citationIdentifying Multiple Populations in M71 Using CN
Gerber, J. M., Friel, E. D., & Vesperini, E. (2020) · The Astronomical Journal · doi:10.3847/1538-3881/ab607e · Cited by 12
The chemical compositions of multiple stellar populations in the globular cluster NGC 2808
Carlos, M., Marino, A. F., Milone, A. P., Dondoglio, E., Jang, S., Legnardi, M. V., Mohandasan, A., Cordoni, G., Lagioia, E. P., Amarsi, A. M., et al. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac3561 · Cited by 12
On the Chemical Abundances of Miras in Clusters: V1 in the Metal-rich Globular NGC 5927*
D’Orazi, V., Magurno, D., Bono, G., Matsunaga, N., Braga, V. F., Elgueta, S. S., Fukue, K., Hamano, S., Inno, L., Kobayashi, N., et al. (2018) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aab100 · Cited by 11
Self-citationSlowly Cooling White Dwarfs in NGC 6752
Chen, J., Ferraro, F. R., Cadelano, M., Salaris, M., Lanzoni, B., Pallanca, C., Althaus, L. G., Cassisi, S., & Dalessandro, E. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac7a45 · Cited by 11
Lee, J.-W. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab3d34 · Cited by 11
AGB subpopulations in the nearby globular cluster NGC 6397
MacLean, B. T., Campbell, S. W., Silva, G. M. D., Lattanzio, J. C., D’Orazi, V., Cottrell, P. L., Momany, Y., & Casagrande, L. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx3217 · Cited by 10
Self-citationMucciarelli, A., Lapenna, E., Lardo, C., Bonifacio, P., Ferraro, F. R., & Lanzoni, B. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/aaf3a4 · Cited by 9
Maximum helium content of multiple populations in the globular cluster NGC 6752
Martins, F., Chantereau, W., & Charbonnel, C. (2021) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/202140800/pdf · Cited by 9
Towards 21st century stellar models: Star clusters, supercomputing and asteroseismology
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Self-citationIntegrated Spectra of Milky Way Globular Clusters
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Maximum helium content of multiple populations in the globular cluster NGC 6752
Martins, F., Chantereau, W., & Charbonnel, C. (2021) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202140800 · Cited by 7
A photometric study of globular clusters observed by the APOGEE survey
Mészáros, S., García-Hernández, D. A., Cassisi, S., Monelli, M., Szigeti, L., Dell’Agli, F., Derekas, A., Masseron, T., Shetrone, M. D., Stetson, P. B., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx3275 · Cited by 6
The Populations of Carina. I. Decoding the Color–Magnitude Diagram
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Self-citationThe evolutionary state of the red giant star L2 Puppis
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Light Element Abundances and Multiple Populations in M53
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A review of the search for AGB stars
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HIGHLIGHTS OF COMMISSION 37 SCIENCE RESULTS
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The predicted properties of helium-enriched globular cluster progenitors at high redshift
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A stellar mid-life crisis: why do some cluster stars die early?
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Self-citationObservational aspects of globular cluster and halo stars in the GALAH survey
Mohd Saadon, M. H. (2022) · UNSWorks (University of New South Wales, Sydney, Australia) · doi:10.26190/unsworks/22405
Metadata
- Authors
- Campbell, S. W., D’Orazi, V., Yong, D., Constantino, T. N., Lattanzio, J. C., Stancliffe, R. J., Angelou, G. C., Wylie-de Boer, E. C., & Grundahl, F.
- Affiliations
- Monash University (AU)
- Australian National University (AU)
- Aarhus University (DK)
- Corresponding author
- Campbell, Simon W.
- ORCID
- Venue
- Nature
- Published
- 2013-05-29
- Volume
- 498
- Issue
- 7453
- Pages
- 198-200
- ISSN
- 0028-0836 (ISSN-L)
- 1476-4687
- OpenAlex
- W2014992560
- Cited by
- 81
- References
- 44
- Citations by year
- 2026: 1 · 2025: 1 · 2024: 2 · 2023: 1 · 2022: 4 · 2021: 4 · 2020: 4 · 2019: 6 · 2018: 7 · 2017: 12 · 2016: 11 · 2015: 15 · 2014: 8 · 2013: 5
- FWCI
- 7.01
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Nature (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- RePEc: Research Papers in Economics (submittedVersion)
- Cineca Institutional Research Information System (Tor Vergata University) (submittedVersion)
- ANU Open Research (Australian National University) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Keywords
- globular clusters, NGC 6752, second-generation stars, first-generation stars, sodium abundance, asymptotic giant branch, stellar evolution, red giant branch, stellar populations
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