activity
20122023
most citedSuper and massive AGB stars - IV. Final fates - Initial to final mass relation

261 citations · 1.3k across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.SR2023★ 17 cited

Aluminium-26 from massive binary stars III. Binary stars up to core-collapse and their impact on the early Solar System

Hannah E. Brinkman, C. L. Doherty, M. Pignatari +2

Many of the short-lived radioactive nuclei that were present in the early Solar System can be produced in massive stars. In the first paper in this series (Brinkman et al. 2019), w…

astro-ph.SR2022★ 14 cited

Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds. II: Spectroscopic and Environmental Analysis of Thorne-Żytkow Object and Super-AGB Star Candidates

Anna J. G. O'Grady, Maria R. Drout, B. M. Gaensler +9

In previous work we identified a population of 38 cool and luminous variable stars in the Magellanic Clouds and examined 11 in detail in order to classify them as either Thorne-Żyt…

astro-ph.SR2022★ 9 cited

Nucleosynthetic yields of intermediate-mass primordial to extremely metal-poor stars

P. Gil-Pons, C. L. Doherty, S. W. Campbell +1

Abridged. We aim to better characterise the evolution and fates, and determine updated nucleosynthetic yields of intermediate-mass stars between primordial and EMP metallicity (Z=1…

astro-ph.SR2022

The RADIOSTAR Project

Maria Lugaro, Benoit Côté, Marco Pignatari +12

Radioactive nuclei are the key to understanding the circumstances of the birth of our Sun because meteoritic analysis has proven that many of them were present at that time. Their…

astro-ph.SR2021★ 5 cited

First models of s process in AGB stars of solar metallicity for the stellar evolutionary code ATON with a novel stable explicit numerical solver

A. Yagüe López, D. A. García-Hernández, P. Ventura +4

Aims. We describe the first s-process post-processing models for asymptotic giant branch (AGB) stars of masses 3, 4 and 5 M at solar metallicity (Z=0.018) computed using the input…

astro-ph.SR2021★ 29 cited

Aluminium-26 from massive binary stars II. Rotating single stars up to core-collapse and their impact on the early Solar System

Hannah E. Brinkman, J. W. den Hartogh, C. L. Doherty +2

Radioactive nuclei were present in the early Solar System, as inferred from analysis of meteorites. Many are produced in massive stars, either during their lives or their final exp…