# Heavy Elements in Stars

@article{Boothroyd2006HeavyEI,
title={Heavy Elements in Stars},
author={A. Boothroyd},
journal={Science},
year={2006},
volume={314},
pages={1690 - 1691}
}
Abundances of elements produced in stars four to eight times the mass of the Sun indicate a different dominant nuclear reaction mechanism than in lower-mass stars.
4 Citations
Origin of the Chemical Elements
• Physics
• 2011
This review provides the necessary background from astrophysics, nuclear, and particle physics to understand the cosmic origin of the chemical elements. It reflects the year 2009 state of the art in
Challenges in nucleosynthesis of trans-iron elements
Nucleosynthesis beyond Fe poses additional challenges not encountered when studying astrophysical processes involving light nuclei. Astrophysical sites and conditions are not well known for some of
Photodisintegration studies ofastrophysically relevant p-nuclei
The majority of the light elements up to iron (Fe) are formed by successive rounds of thermonuclear fusion burning in the stellar interiors. The nuclei heavier than iron (Z>26) are being synthesized
Alpha-induced reaction cross section measurements on $^{151}$Eu for the astrophysical $\gamma$-process
In order to extend the experimental database relevant for the astrophysical -process towards the unexplored heavier mass region, the cross sections of the 151 Eu(�,) 155 Tb and 151 Eu(�,n) 154 Tb

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