Presolar SiC Grains of Type A and B: Their Isotopic Compositions and Stellar Origins

By S. Amari, L. Nittler, E. Zinner, K. Lodders, R. Lewis. 2001

143 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/ff9da01ebdb10d26dabe0c9844639a216570a3b7

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. A. Karakas
2. M. Lugaro
3. L. Nittler
4. F. Ciesla
5. Denton S. Ebel
6. D. Clayton
7. J. Lattanzio
8. M. Busso

In Geophysics

1. Denton S. Ebel
2. A. Karakas
3. L. Nittler

Citations in the corpus

• STELLAR YIELDS FROM METAL-RICH ASYMPTOTIC GIANT BRANCH MODELS (2016, background): “These can be measured in meteoritic stardust grains (e.g. Amari et al. 2001a), Furthermore, the Si isotopic ratios can be measured in AGB stars via molecular lines (e.g., from SiO, Peng et al. 2013).”
• Astrophysics with Presolar Stardust (2004, background): “Fewer then ten grains of SiC and graphite have been reported with isotopic signatures strongly pointing to a nova origin (Amari et al. 2001a, Nittler & Alexander 2003a).”
• Cool Bottom Processes on the Thermally Pulsing Asymptotic Giant Branch and the Isotopic Composition of Circumstellar Dust Grains (2002, background): “They belong to the very small class (6 known) of carbon-rich grains attributed to novae on the basis of C, N, and Si isotopic compositions, and they are not A and B grains (Amari et al. 2001c).”
• Presolar stardust in meteorites : recent advances and scientific frontiers (2003, background): “Isotopic and trace-element data from a large number of A+B grains suggest a connection to J stars and ‘born-again’ AGB stars [46], but the evolution of these stars is unfortunately still poorly understood.”
• Astrophysics with Extraterrestrial Materials (2016, background): “%) of presolar SiC, graphite, silicate, and oxide grains (Amari et al. 2001a, Gyngard et al. 2010b, Leitner et al. 2012), in addition to a few of the 13C-rich grains just discussed (Heck et al. 2007).”
• Condensation of Rocky Material in Astrophysical Environments (2023, methodology): “Condensation calculations using these results as inputs are vital to understanding the origins of interstellar and presolar grains (e.g., Amari et al., 2001; Ebel and Grossman, 2001; cf. review by Lodders and Fegley, 1997).”