Marco Pignatari
0000-0002-9048-6010
University of Hull
187 papers found
Refreshing results…
The Nucleosynthetic Yields of Core-collapse Supernovae: Prospects for the Next Generation of Gamma-Ray Astronomy
Isotopic Signatures of Supernova Nucleosynthesis in Presolar Silicon Carbide Grains of Type AB with Supersolar 14N/15N Ratios
A direct measurement of the 17O(α,γ)21Ne reaction in inverse kinematics and its impact on heavy element production
Enrichment of the Galactic disc with neutron-capture elements: Mo and Ru
Galactic Chemical Evolution of Radioactive Isotopes
Using failed supernovae to constrain the Galactic r-process element production
Neutron Star Mergers Might Not Be the Only Source of r-process Elements in the Milky Way
Enrichment of the Galactic disc with neutron capture elements: Sr
Nucleosynthetic yields from neutron stars accreting in binary common envelopes
Remnants and ejecta of thermonuclear electron-capture supernovae
H-He Shell Interactions and Nucleosynthesis in Massive Population III Stars
Heavy Elements Nucleosynthesis on Accreting White Dwarfs Surface: Seeding the p-Process
Presolar SiC Grains of Type AB with Isotopically Light Nitrogen: Contributions from Supernovae?
Inhomogeneous Chemical Evolution of r-Process Elements in the Galactic Halo
The s process in AGB stars as constrained by a large sample of barium stars
Corrigendum to “Iron and nickel isotope compositions of presolar silicon carbide grains from supernovae” [Geochim. Cosmochim. Acta 221 (2018) 127–144]
The composition of Barium stars and the s-process in AGB stars
NuGrid stellar data set – II. Stellar yields from H to Bi for stellar models with MZAMS = 1–25 M⊙ and Z = 0.0001–0.02
The impact of (n,γ) reaction rate uncertainties of unstable isotopes nearN= 50 on the i-process nucleosynthesis in He-shell flash white dwarfs
i-process Contribution of Rapidly Accreting White Dwarfs to the Solar Composition of First-peak Neutron-capture Elements
Missing publications? Search for publications with a matching author name.