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astro-ph.SR2026

V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories

James Munday, Antonio C. Rodriguez, Nicole Reindl +23

The AM CVn class includes mass transferring, ultra-compact double white dwarf binaries with orbital periods on the timescale of minutes. A long-standing puzzle is that none of the…

astro-ph.SR2026

Mode Instability and a Massive, Isolated Outburst in the Pulsating White Dwarf GD 1212

J. J. Hermes, Keaton J. Bell, Andrew H. Dublin +8

We analyze a large brightening event that lasted for roughly half a day in the pulsating hydrogen-atmosphere white dwarf GD 1212 during K2 Campaign 12 of the extended Kepler missio…

astro-ph.SR2026

Improved Stark Broadened Profiles for Neutral Helium Lines Using Computer Simulations

Patrick Tremblay, Alain Beauchamp, Pierre Bergeron +1

The study of Stark broadening of neutral helium lines, despite significant advances over recent decades, has not led to updated large grids of helium line profiles relevant to the…

astro-ph.SR2025

J-PLUS: Understanding outlier white dwarfs in the third data release via dimensionality reduction

C. López-Sanjuan, P. -E. Tremblay, A. del Pino +20

We present the white dwarf catalog derived from the third data release of the Javalambre Photometric Local Universe Survey (J-PLUS DR3), which covers 3284 deg2 using 12 optical fil…

astro-ph.SR2024

J-PLUS: The fraction of calcium white dwarfs along the cooling sequence

C. López-Sanjuan, P. -E. Tremblay, M. W. O'Brien +24

We used the Javalambre Photometric Local Universe Survey (J-PLUS) DR2 photometry in twelve optical bands over 2176 deg2 to estimate the fraction of white dwarfs with presence of Ca…