The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
Y 2 Isochrones with an Improved Core Overshoot Treatment
Open accessAbstract
Convective core overshoot affects stellar evolution rates and the dating of stellar populations. In this paper, we provide a patch to the Y 2 isochrones with an improved treatment of convective core overshoot. The new tracks cover the transition mass range from no convective core to a fully developed convective core. We compare the improved isochrones to CMDs of a few well-observed open star clusters in the Galaxy and the Large Magellanic Cloud. Finally, we discuss future prospects for improving the treatment of core overshoot with the help of asteroseismology.
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Cites
Low-temperature Rosseland opacities
Alexander, D. R., & Ferguson, J. W. (1994) · The Astrophysical Journal · doi:10.1086/175039 · Cited by 1,161
Cited by
MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
Choi, J., Dotter, A., Conroy, C., Cantiello, M., Paxton, B., & Johnson, B. D. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/823/2/102 · Cited by 2,922
PLANETARY CANDIDATES OBSERVED BY KEPLER . III. ANALYSIS OF THE FIRST 16 MONTHS OF DATA
Batalha, N. M., Rowe, J. F., Bryson, S. T., Barclay, T., Burke, C. J., Caldwell, D. A., Christiansen, J. L., Mullally, F., Thompson, S. E., Brown, T. M., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/204/2/24 · Cited by 1,042
Neutron-Capture Elements in the Early Galaxy
Sneden, C., Cowan, J. J., & Gallino, R. (2008) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.46.060407.145207 · Cited by 968
THE OCCURRENCE RATE OF SMALL PLANETS AROUND SMALL STARS
Dressing, C. D., & Charbonneau, D. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/767/1/95 · Cited by 749
Pecaut, M. J., Mamajek, E. E., & Bubar, E. J. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/746/2/154 · Cited by 564
“While a choice of different theoretical tracks vary this disagreement slightly (e.g., D’Antona & Mazzitelli (1997), Siess et al. (2000), Demarque et al. (2004)) the disparity is at least ∼0.4 dex at spectral type F3, which corresponds to a factor of & 2.5 in luminosity, or about 1 mag.”
BackgroundMethodInfluential
Metadata
- Authors
- Demarque, P., Woo, J., Kim, Y., & Yi, S. K.
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Published
- 2004-12
- Volume
- 155
- Issue
- 2
- Pages
- 667-674
- ISSN
- 0067-0049 (ISSN-L)
- 1538-4365
- OpenAlex
- W2039452097
- Cited by
- 977
- References
- 1
- FWCI
- 12.41
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Demarque, P., Woo, J., Kim, Y., & Yi, S. K. (2004). Y 2 Isochrones with an Improved Core Overshoot Treatment. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/424966
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