activity
20192025
most citedThe chemical evolution of the solar neighbourhood for planet-hosting stars

15 citations · 44 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025

Trans-Fe elements from Type Ia Supernovae. I. Heavy element nucleosynthesis during the formation of near-Chandrasekhar white dwarfs

Umberto Battino, James Keegans, Megan Allen +9

Type Ia supernovae (SNIa) are thermonuclear explosions of white dwarfs in binary systems. They are central to galactic chemical evolution and serve as standardizable candles in cos…

astro-ph.SR2025★ 6 cited

Using chemical evolution models of the Milky Way disk to constrain Type Ia supernova progenitors

T. C. L. Trueman, M. Pignatari, B. Cseh +3

Thermonuclear explosions of carbon-oxygen white dwarfs as Type Ia supernovae (SNe Ia) play a significant role in the galactic chemical evolution (GCE) of the Milky Way. However, a…

astro-ph.GA2023★ 15 cited

The chemical evolution of the solar neighbourhood for planet-hosting stars

Marco Pignatari, Thomas C. L. Trueman, Kate A. Womack +13

Theoretical physical-chemical models for the formation of planetary systems depend on data quality for the Sun's composition, that of stars in the solar neighbourhood, and of the e…

astro-ph.HE2023★ 15 cited

Type Ia Supernova Nucleosynthesis: Metallicity-Dependent Yields

James D Keegans, Marco Pignatari, Richard J Stancliffe +7

Type Ia supernova explosions (SNIa) are fundamental sources of elements for the chemical evolution of galaxies. They efficiently produce intermediate-mass (with Z between 11 and 20…

physics.ed-ph2021

Project ThaiPASS: International Outreach Blending Astronomy and Python

James D. Keegans, Richard J. Stancliffe, Lawrence E. Bilton +8

(ThaiPASS), a collaborative project comprising UK and Thai institutions and assess its impact and possible application to scho…

astro-ph.SR2019★ 8 cited

Nucleosynthetic Yields from Neutron Stars Accreting in Binary Common Envelopes

James D. Keegans, Chris L. Fryer, Samuel W. Jones +6

Massive-star binaries can undergo a phase where one of the two stars expands during its advanced evolutionary stage as a giant and envelops its companion, ejecting the hydrogen env…