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astro-ph.SR2025

Circumstellar interaction in the extreme white dwarf merger remnant ZTF\,J1901+1458: A new class of white dwarf merger remnants with X-ray emission

Aayush Desai, Ilaria Caiazzo, Stephane Vennes +31

Double degenerate white dwarf (WD) mergers can exhibit extreme magnetic fields exceeding G and rapid rotation, but their spectral-energy distributions and high-energy emis…

astro-ph.SR2025

Double White Dwarf Binaries in SDSS-V DR19 : A catalog of DA white dwarf binaries and constraints on the binary population

Gautham Adamane Pallathadka, Vedant Chandra, Nadia L. Zakamska +17

The fifth-generation Sloan Digital Sky Survey (SDSS-V) includes the first large-scale spectroscopic survey of white dwarfs (WDs) in the era of Gaia parallaxes. SDSS-V collects mult…

astro-ph.SR2025

A hot white dwarf merger remnant revealed by an ultraviolet detection of carbon

Snehalata Sahu, Antoine Bédard, Boris T. Gänsicke +7

Atmospheric carbon has been detected in the optical spectra of six hydrogen-rich ultra-massive white dwarfs, revealing large carbon abundances (log C/H > 0.5) attributable to th…

astro-ph.SR2025

The DBL Survey II: towards a mass-period distribution of double white dwarf binaries

James Munday, Ingrid Pelisoli, Pier-Emmanuel Tremblay +14

Double white dwarf binaries are an important remnant of binary evolution as they are possible type Ia supernova progenitors and strong sources of gravitational waves in the low-fre…

astro-ph.SR2025

A half-ring of ionized circumstellar material trapped in the magnetosphere of a white dwarf merger remnant

Andrei A. Cristea, Ilaria Caiazzo, Tim Cunningham +31

Many white dwarfs are observed in compact double white dwarf binaries and, through the emission of gravitational waves, a large fraction are destined to merge. The merger remnants…

astro-ph.SR2025

Double White Dwarf Binaries in SDSS-V DR19 : The discovery of a rare DA+DQ white dwarf binary with 31 hour orbital period

Gautham Adamane Pallathadka, Vedant Chandra, Boris T. Gansicke +13

Binaries of two white dwarfs (WDs) are an important class of astrophysical objects that are theorized to lead to Type Ia supernovae and are also used to gain insight into complex p…