Origin of meteoritic stardust unveiled by a revised proton-capture rate of 17 O
2017
Isotopic analyses of stardust have yet to single out a specific stellar origin for it. A revision of the proton-capture rate of 17O has helped to identify intermediate mass stars (4–8 solar masses) as the source of a large fraction of meteoritic stardust.
- Correction
- Source
- Cite
- Save
- Machine Reading By IdeaReader
37
References
53
Citations
NaN
KQI