M. Pignatari

Spectacular Nucleosynthesis from Early Massive Stars

Type Ia Supernova Nucleosynthesis: Metallicity-dependent Yields

Deep Underground Laboratory Measurement of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>13</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><m

Remnants and ejecta of thermonuclear electron-capture supernovae

The neutron capture process in the He shell in core-collapse supernovae: Presolar silicon carbide grains as a diagnostic tool for nuclear astrophysics

The production of proton-rich isotopes beyond iron: The γ-process in stars

CARBON-RICH PRESOLAR GRAINS FROM MASSIVE STARS: SUBSOLAR ¹² C/ ¹³ C AND ¹⁴ N/ ¹⁵ N RATIOS AND THE MYSTERY OF ¹⁵ N

New insights on Ba overabundance in open clusters.★ Evidence for the intermediate neutron-capture process at play?

BARIUM ISOTOPIC COMPOSITION OF MAINSTREAM SILICON CARBIDES FROM MURCHISON: CONSTRAINTS FOR<i>s</i>-PROCESS NUCLEOSYNTHESIS IN ASYMPTOTIC GIANT BRANCH STARS

High-resolution abundance analysis of red giants in the globular cluster NGC 6522

MESA and NuGrid simulations of classical novae: CO and ONe nova nucleosynthesis

SILICON CARBIDE GRAINS OF TYPE C PROVIDE EVIDENCE FOR THE PRODUCTION OF THE UNSTABLE ISOTOPE ³² Si IN SUPERNOVAE

The effect of 12C +12C rate uncertainties on the evolution and nucleosynthesis of massive stars