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Current challenges in the physics of white dwarf stars
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 …
challenging problems whose solution requires advanced theories of dense matter, state-of …
Modules for experiments in stellar astrophysics (MESA): time-dependent convection, energy conservation, automatic differentiation, and infrastructure
We update the capabilities of the open-knowledge software instrument Modules for
Experiments in Stellar Astrophysics (MESA). The new auto _ diff module implements …
Experiments in Stellar Astrophysics (MESA). The new auto _ diff module implements …
A catalogue of white dwarfs in Gaia EDR3
We present a catalogue of white dwarf candidates selected from Gaia Early Data Release 3
(EDR3). We applied several selection criteria in absolute magnitude, colour, and Gaia …
(EDR3). We applied several selection criteria in absolute magnitude, colour, and Gaia …
[HTML][HTML] The Gaia white dwarf revolution
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 …
research. These stellar remnants constitute 5%–7% of the local stellar population in volume …
Buoyant crystals halt the cooling of white dwarf stars
White dwarfs are stellar remnants devoid of a nuclear energy source, gradually cooling over
billions of years, and eventually freezing into a solid state from the inside out,. Recently, it …
billions of years, and eventually freezing into a solid state from the inside out,. Recently, it …
Skye: A differentiable equation of state
Stellar evolution and numerical hydrodynamics simulations depend critically on access to
fast, accurate, thermodynamically consistent equations of state. We present Skye, a new …
fast, accurate, thermodynamically consistent equations of state. We present Skye, a new …
Magnetic field breakout from white dwarf crystallization dynamos
ABSTRACT A convective dynamo operating during the crystallization of white dwarfs is one
of the promising channels to produce their observed strong magnetic fields. Although the …
of the promising channels to produce their observed strong magnetic fields. Although the …
Carbon–oxygen phase separation in modules for experiments in stellar astrophysics (MESA) white dwarf models
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 …
evolution software Modules for Experiments in Stellar Astrophysics (MESA) by implementing …
Evolutionary models for the remnant of the merger of two carbon-oxygen core white dwarfs
We construct evolutionary models of the remnant of the merger of two carbon-oxygen (CO)
core white dwarfs (WDs). With total masses in the range 1–2 M⊙, these remnants may either …
core white dwarfs (WDs). With total masses in the range 1–2 M⊙, these remnants may either …
22Ne phase separation as a solution to the ultramassive white dwarf cooling anomaly
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 …
detailed tests of the predictions of white dwarf cooling models. Significant discrepancies …