178 citations · 629 across the 10 of their papers we have counts for
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astro-ph.SR2013★ 17 cited
Systematic and correlated nuclear uncertainties in the i-process at the neutron shell closure N = 82
M. G. Bertolli, F. Herwig, M. Pignatari +1
Nuclear astrophysics simulations aiming to study the origin of the elements in stars require a multitude of nuclear physics input. Both systematic model dependent and statistically…
astro-ph.SR2013★ 54 cited
Production of carbon-rich presolar grains from massive stars
M. Pignatari, M. Wiescher, F. X. Timmes +6
About a year after core collapse supernova, dust starts to condense in the ejecta. In meteorites, a fraction of C-rich presolar grains (e.g., silicon carbide (SiC) grains of Type-X…