Realistic models of the Galactic double white dwarf (DWD) population are crucial for testing
and quantitatively defining the science objectives of the Laser Interferometer Space Antenna …

Abstract AM Canum Venaticorum (AM CVn) systems are ultracompact binaries where a
white dwarf accretes from a helium-rich degenerate or semidegenerate donor. Some AM …

ABSTRACT AM CVn systems are ultra-compact, hydrogen-depleted, and helium-rich,
accreting binaries with degenerate or semidegenerate donors. We report the discovery of …

This review highlights the role of the Gaia space mission in transforming white dwarf
research. These stellar remnants constitute 5%–7% of the local stellar population in volume …

We present the discovery of the eclipsing double white dwarf (WD) binary WDJ 022558.21−
692025.38 that has an orbital period of 47.19 min. Following identification with the Transiting …

Galactic short-period close white dwarf binaries (CWDBs) are important objects for space-
borne gravitational-wave (GW) detectors in the millihertz frequency bands. Due to the …

We present a study of 323 photometrically variable young stellar objects that are likely
members of the North America and Pelican nebulae star-forming region. To do so, we utilize …

In a search for eclipsing white dwarfs using the Zwicky Transient Facility lightcurves, we
identified a deep eclipsing white dwarf with an orbital period of 10.4 hr and an undetected …

Context. Ultracompact cataclysmic variables (CVs) of the AM CVn type are deemed to be
important verification sources for the future space gravitational wave detectors such as the …

Compact-object binaries including a white dwarf component are unique among gravitational-
wave sources because their evolution is governed not just by general relativity and tides, but …