White dwarfs are a class of stars with unique physical properties. They present many
challenging problems whose solution requires advanced theories of dense matter, state-of …

Yearslong time series of high-precision brightness measurements have been assembled for
thousands of stars with telescopes operating in space. Such data have allowed astronomers …

We present a catalogue of white dwarf candidates selected from the second data release of
Gaia (DR2). We used a sample of spectroscopically confirmed white dwarfs from the Sloan …

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), also known as
the Guoshoujing Telescope, is a major national scientific facility for astronomical research …

White dwarfs represent the final state of evolution for most stars,–. Certain classes of white
dwarfs pulsate,, leading to observable brightness variations, and analysis of these variations …

Stars are extremely important astronomical objects that constitute the pillars on which the
Universe is built, and as such, their study has gained increasing interest over the years …

We enhance the treatment of crystallization for models of white dwarfs (WDs) in the stellar
evolution software Modules for Experiments in Stellar Astrophysics (MESA) by implementing …

We present new cooling models for carbon–oxygen white dwarfs (WDs) with both H-and He-
atmospheres, covering the whole relevant mass range, to extend our updated basti (a Bag of …

The precise astrometric measurements of the Gaia Data Release 2 have opened the door to
detailed tests of the predictions of white dwarf cooling models. Significant discrepancies …

We report on studies of classical nova (CN) explosions where we follow the evolution of
thermonuclear runaways (TNRs) on carbon–oxygen (CO) white dwarfs (WDs). We vary both …