The DOI matches its Crossref record; 137 of the 137 references it cites were found in a registry or an index.
Astrophysics with Presolar Stardust
Abstract
▪ Abstract Meteorites and interplanetary dust particles contain presolar stardust grains: solid samples of stars that can be studied in the laboratory. The stellar origin of the grains is indicated by enormous isotopic ratio variations compared with Solar System materials, explainable only by nuclear reactions occurring in stars. Known presolar phases include diamond, SiC, graphite, Si 3 N 4, Al 2 O 3, MgAl 2 O 4, CaAl 12 O 19, TiO 2, Mg(Cr,Al)2 O 4, and most recently, silicates. Subgrains of refractory carbides (e.g., TiC), and Fe-Ni metal have also been observed within individual presolar graphite grains. We review the astrophysical implications of these grains for the sciences of nucleosynthesis, stellar evolution, grain condensation, and the chemical and dynamic evolution of the Galaxy. Unique scientific information derives primarily from the high precision (in some cases <1%) of the measured isotopic ratios of large numbers of elements in single stardust grains. Stardust science is just now reaching maturity and will play an increasingly important role in nucleosynthesis applications.
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Cites
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Cited by
The Discovery and Analysis of Very Metal-Poor Stars in the Galaxy
Beers, T. C., & Christlieb, N. (2005) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.42.053102.134057 · Cited by 1,223
The Chemical Composition of Comets—Emerging Taxonomies and Natal Heritage
Mumma, M. J., & Charnley, S. B. (2011) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081309-130811 · Cited by 916
High‐Resolution Submillimeter Constraints on Circumstellar Disk Structure
Andrews, S. M., & Williams, J. P. (2007) · The Astrophysical Journal · doi:10.1086/511741 · Cited by 426
Dust formation and survival in supernova ejecta
Bianchi, S., & Schneider, R. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.11829.x · Cited by 401
Can Extra Mixing in RGB and AGB Stars Be Attributed to Magnetic Mechanisms?
Busso, M., Wasserburg, G. J., Nollett, K. M., & Calandra, A. (2007) · The Astrophysical Journal · doi:10.1086/522616 · Cited by 150
Metadata
- Authors
- Clayton, D. D., & Nittler, L. R.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2004-09-22
- Volume
- 42
- Issue
- 1
- Pages
- 39-78
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2104433774
- Cited by
- 295
- References
- 137
- FWCI
- 2.17
- Type
- journal article
- Language
- en
- Open access
- closed
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