Silicon Isotopic Composition of Mainstream Presolar SiC Grains Revisited: The Impact of Nuclear Reaction Rate Uncertainties
Presolar grains are stardust particles that condensed in the ejecta or in the outflows of dying stars and can today be extracted from meteorites. They recorded the nucleosynthetic fingerprint of their parent stars and thus serve as valuable probes of these astrophysical sites. The most common types...
Saved in:
| Main Authors: | Hung Kwan Fok, Marco Pignatari, Benoît Côté, Reto Trappitsch |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
|
| Series: | The Astrophysical Journal Letters |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/2041-8213/ad91ab |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The Impact of Initial Composition on Massive Star Evolution and Nucleosynthesis
by: Christopher West, et al.
Published: (2025-01-01) -
New Stellar Parameters, Metallicities, and Elemental Abundance Ratios for 311 Metal-poor Stars
by: Sanil Mittal, et al.
Published: (2025-01-01) -
Searching for R-process-enhanced Stars in the LAMOST Survey. II. Two New r-II Stars in the Milky Way Disk
by: Xiao-Jin Xie, et al.
Published: (2025-01-01) -
The Scale of Stellar Yields: Implications of the Measured Mean Iron Yield of Core Collapse Supernovae
by: David H. Weinberg, et al.
Published: (2024-01-01) -
Iron Snails: Nonequilibrium Dynamics and Spiral Abundance Patterns
by: Neige Frankel, et al.
Published: (2025-01-01)