activity
20092026
most citedSpectroscopic Analysis of DA White Dwarfs: Stark Broadening of Hydrogen Lines Including Non-Ideal Effects

376 citations · 1.5k across the 46 of their papers we have counts for

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13 papers · 1 filter

astro-ph.IM2025

The Future of Evolved Planetary Systems

Roberto Raddi, Anna F. Pala, Alberto Rebassa-Mansergas +19

Understanding the formation, evolution, and chemical diversity of exoplanets are now central areas of astrophysics research. White dwarfs provide a uniquely sensitive laboratory fo…

astro-ph.SR2025

Re-evaluating Lyman wing opacities and the low mass-problem in cool white dwarfs

Snehalata Sahu, Pier-Emmanuel Tremblay, Detlev Koester +4

Gaia observations have reignited interest in the optical and ultraviolet (UV) opacity problems of cool white dwarfs ( K), which were thought to be resolved n…

astro-ph.SR2025

The White Dwarf Initial-Final Mass Relation from Open Clusters in Gaia DR3

David R. Miller, Ilaria Caiazzo, Jeremy Heyl +6

The initial-final mass relation (IFMR) links a star's birth mass to the mass of its white dwarf (WD) remnant, providing key constraints on stellar evolution. Open clusters offer th…

astro-ph.EP2025

Exogeological inferences from white dwarf pollutants: the impact of stellar physics

Andrew M. Buchan, Pier-Emmanuel Tremblay, Antoine Bédard +2

Many white dwarfs have accreted material from their own planetary systems. These objects can be used to infer the composition of exoplanetary material and identify evidence for key…

astro-ph.SR2025

Assessing the star formation history of all-sky and part-sky 100pc white dwarf samples

Emily K. Roberts, Pier-Emmanuel Tremblay, Antoine Bédard

Thanks to Gaia and large-scale spectroscopic follow-up surveys (4MOST, DESI, WEAVE, SDSS-V), it is now possible to build representative and minimally biased samples of the local wh…

astro-ph.SR2025

MESA Isochrones and Stellar Tracks (MIST) III. The White Dwarf Cooling Sequence

Evan B. Bauer, Aaron Dotter, Charlie Conroy +3

We present a substantial update to the MESA Isochrones and Stellar Tracks (MIST) library, extending the MIST model grids and isochrones down the white dwarf (WD) cooling sequence w…