collaborators

7 papers

astro-ph.SR2026

A Detailed Model Atmosphere Analysis of Cool White Dwarfs in DESI DR1

Mukremin Kilic, Pierre Bergeron, Simon Blouin +9

We present a detailed model atmosphere analysis of cool white dwarfs in the Dark Energy Spectroscopic Instrument Data Release 1 (DESI DR1). Our sample includes 25,642 unique target…

astro-ph.SR2026

A Detailed Model Atmosphere Analysis of Hot White Dwarfs in DESI DR1

Mukremin Kilic, Pierre Bergeron, Adam Moss +6

We present a detailed model atmosphere analysis of hot white dwarfs in the Dark Energy Spectroscopic Instrument (DESI) Data Release 1. Our sample includes 19,321 unique targets wit…

astro-ph.SR2026

White Dwarf Merger Remnants with Cooling Delays on the Q Branch Lack Strong Magnetism

Lou Baya Ould Rouis, J. J. Hermes, Joseph A. Guidry +8

A population of anomalous ultra-massive white dwarfs discovered with Gaia, often referred to as the Q branch, show high (multi-Gyr) cooling delays produced by exotic physical mecha…

astro-ph.SR2025

Comparison of Ne-22 core and shell distilled WD detonations in AREPO

Uri Pierre Burmester, Lilia Ferrario, Ivo R. Seitenzahl +1

We present three-dimensional hydrodynamical simulations of detonations in white dwarfs that have undergone distillation during crystall…

astro-ph.SR2025

JWST imaging of omega Centauri: II. Evidence for a split white dwarf cooling sequence in the near-infrared

M. Scalco, M. Salaris, L. R. Bedin +11

We present a detailed analysis of the white dwarf cooling sequence (WD CS) in omega Centauri based on combined Hubble Space Telescope (HST) and JWST observations. Our analysis conf…

astro-ph.SR2025

The Fraction of Distilled White Dwarfs with Long-Lived Habitable Zones

Manuel Barrientos, Mukremin Kilic, Simon Blouin +3

After carbon and oxygen, Ne is the most abundant element in white dwarf interiors. As C/O white dwarfs (WDs) crystallize, they are predicted to go through a distillation pro…