Type Ia supernovae (SNIa) are luminous stellar explosions which mark the fatal disruption of white dwarfs in a binary system. They are the major producers of Iron group elements in the solar system and also give relevant contribution to the alpha-elements Silicon, Solfur, Calcium and Titanium. Within specific conditions SNIa may also produce about 30 proton-rich isotopes heavier than iron. It is controversial what is the relevance of this p-process component for the abundance of these isotopes in the Galaxy and in our solar system. Its efficiency depends on the products of neutron capture processes active during the accretion phase to reach the Chandrasekhar mass. The aim of this thesis is to provide for the first time comprehensive stellar...
© 2019, Springer Nature Switzerland AG. The production of the proton-rich isotopes beyond iron that ...
[abridged] We study the s-process in AGB stars using three different stellar evolutionary models com...
We present a review of nucleosynthesis in AGB stars outlining the development of theoretical models ...
© The Author(s) 2020. Published by Oxford University Press on behalf of The Royal Astronomical Socie...
The origin of the proton-rich trans-iron isotopes in the Solar system is still uncertain. Single-deg...
The production of the p-process nuclides that we observe today in the Solar Systemis still uncertain...
The production of the neutron-capture isotopes beyond iron that we observe today in the Solar system...
The production of the neutron-capture isotopes beyond iron that we observe today in the Solar system...
Many nucleosynthesis and mixing processes of low-mass stars as they evolve from the Main Sequence to...
© 2019 Oxford University Press. All rights reserved. The production of the neutron-capture isotopes ...
[abridged] We study the s-process in AGB stars using three different stellar evolutionary models com...
Asymptotic Giant Branch (AGB) stars play a key role in the chemical evolution of galaxies. These sta...
This thesis is about the evolution of stars, specifically about the final fate of stars at the borde...
© 2019, Springer Nature Switzerland AG. The production of the proton-rich isotopes beyond iron that ...
Elements heavier than iron are almost entirely produced in stars through neutron captures and radio...
© 2019, Springer Nature Switzerland AG. The production of the proton-rich isotopes beyond iron that ...
[abridged] We study the s-process in AGB stars using three different stellar evolutionary models com...
We present a review of nucleosynthesis in AGB stars outlining the development of theoretical models ...
© The Author(s) 2020. Published by Oxford University Press on behalf of The Royal Astronomical Socie...
The origin of the proton-rich trans-iron isotopes in the Solar system is still uncertain. Single-deg...
The production of the p-process nuclides that we observe today in the Solar Systemis still uncertain...
The production of the neutron-capture isotopes beyond iron that we observe today in the Solar system...
The production of the neutron-capture isotopes beyond iron that we observe today in the Solar system...
Many nucleosynthesis and mixing processes of low-mass stars as they evolve from the Main Sequence to...
© 2019 Oxford University Press. All rights reserved. The production of the neutron-capture isotopes ...
[abridged] We study the s-process in AGB stars using three different stellar evolutionary models com...
Asymptotic Giant Branch (AGB) stars play a key role in the chemical evolution of galaxies. These sta...
This thesis is about the evolution of stars, specifically about the final fate of stars at the borde...
© 2019, Springer Nature Switzerland AG. The production of the proton-rich isotopes beyond iron that ...
Elements heavier than iron are almost entirely produced in stars through neutron captures and radio...
© 2019, Springer Nature Switzerland AG. The production of the proton-rich isotopes beyond iron that ...
[abridged] We study the s-process in AGB stars using three different stellar evolutionary models com...
We present a review of nucleosynthesis in AGB stars outlining the development of theoretical models ...