888 citations · 7k across the 96 of their papers we have counts for
40 papers · 1 filter
Ejecta clumps revealed by study of reverse-shocked ejecta through MUSE integral field spectroscopy of SNR 0509-67.5
Priyam Das, Ivo Seitenzahl, J. Martin Laming +3
We report the discovery of a spatially resolved clumpy ejecta structure in the reverse-shocked ejecta of SNR 0509-67.5, revealed through multiple faint and broad forbidden coronal…
Deep MUSE observations of SNR 0509-67.5 reveal a double degenerate merger progenitor
Priyam Das, Ivo R. Seitenzahl, Gilles Ferrand +5
Deep MUSE observations of SNR 0509-67.5 reveal that the coronal [Fe\,\textsc{xiv}] 5303 emission line appears with either one or two velocity components across the entire…
Observational constraints on the origin of the elements. IX. 3D NLTE abundances of metals in the context of Galactic Chemical Evolution Models and 4MOST
Nicholas Storm, Maria Bergemann, Philipp Eitner +8
Historically, various methods have been employed to understand the origin of the elements, including observations of elemental abundances which have been compared to Galactic Chemi…
Population synthesis of hot-subdwarf B stars with COMPAS: parameter variations and a prescription for hydrogen-rich shells
Nicolás Rodríguez-Segovia, Ashley J. Ruiter, Ivo R. Seitenzahl
Subdwarf B stars are a well-known class of hot, low-mass stars thought to be formed through interactions in stellar binary systems. While different formation channels for subdwarf…
Type Ia supernova progenitors: a contemporary view of a long-standing puzzle
Ashley J. Ruiter, Ivo R. Seitenzahl
Type Ia supernovae (SNe Ia) are runaway thermonuclear explosions in white dwarfs that result in the disruption of the white dwarf star, and possibly its nearby stellar companion. S…
AREPO White Dwarf merger simulations resulting in edge-lit detonation and run-away hypervelocity companion
Uri Pierre Burmester, Lilia Ferrario, Rüdiger Pakmor +3
We present a series of high-resolution simulations generated with the moving-mesh code AREPO to model the merger of a carbon-oxygen primary white dwarf wi…