activity
20242026
collaborators

8 papers

astro-ph.SR2026

White dwarfs within 13 pc: Insights from ultraviolet spectroscopy

Mairi W. O'Brien, Pier-Emmanuel Tremblay, Boris T. Gaensicke +9

We present a comprehensive multi-wavelength spectroscopic and photometric analysis of the 44 confirmed white dwarfs within 13 pc of the Sun. Combining flux-calibrated ultraviolet (…

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.SR2025

Transiting Planetary Debris near the Roche Limit of a White Dwarf on a 4.97hr Orbit -- and its Vanishing

Joseph A. Guidry, Zachary P. Vanderbosch, J. J. Hermes +9

We present the discovery of deep, irregular, periodic transits towards the white dwarf ZTFJ19444557 using follow-up time-series photometry and spectroscopy from Palomar, Kec…

astro-ph.SR2025

A ZTF Search for Circumstellar Debris Transits in White Dwarfs: Six New Candidates, one with Gas Disk Emission, identified in a Novel Metric Space

Soumyadeep Bhattacharjee, Zachary P. Vanderbosch, Mark A. Hollands +13

White dwarfs (WDs) showing transits from orbiting planetary debris provide significant insights into the structure and dynamics of debris disks. This is a rare class of objects wit…

astro-ph.SR2025

The dearth of high-mass hydrogen-atmosphere metal-polluted white dwarfs within 40 pc

Tim Cunningham, Pier-Emmanuel Tremblay, Mairi O'Brien +7

We present a population synthesis model which addresses the different mass distributions of the metal-polluted and non-metal-polluted hydrogen-atmosphere white dwarfs identified in…

astro-ph.SR2025

Two almost planetary mass survivors of common envelope evolution

S. G. Parsons, A. J. Brown, S. L. Casewell +19

White dwarfs are often found in close binaries with stellar or even substellar companions. It is generally thought that these compact binaries form via common envelope evolution, t…