Buoyant crystals halt the cooling of white dwarf stars

A Bédard, S Blouin, S Cheng - Nature, 2024 - nature.com
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 …

Magnetic field breakout from white dwarf crystallization dynamos

D Blatman, S Ginzburg - Monthly Notices of the Royal …, 2024 - academic.oup.com
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 …

The 40 pc sample of white dwarfs from Gaia

MW O'Brien, PE Tremblay, BL Klein… - Monthly Notices of …, 2024 - academic.oup.com
We present a comprehensive overview of a volume-complete sample of white dwarfs
located within 40 pc of the Sun, a significant proportion of which were detected in Gaia Data …

An emerging and enigmatic spectral class of isolated DAe white dwarfs

AK Elms, PE Tremblay, BT Gänsicke… - Monthly Notices of …, 2023 - academic.oup.com
Two recently discovered white dwarfs, WD J041246. 84+ 754942.26 and WD J165335. 21−
100116.33, exhibit Hα and Hβ Balmer line emission similar to stars in the emerging DAHe …

Period bouncers as detached magnetic cataclysmic variables

MR Schreiber, D Belloni, J Van Roestel - Astronomy & Astrophysics, 2023 - aanda.org
Context. The general prediction that more than half of all cataclysmic variables (CVs) have
evolved past the period minimum is in strong disagreement with observational surveys …

Main sequence dynamo magnetic fields emerging in the white dwarf phase

M Camisassa, JR Fuentes, MR Schreiber… - Astronomy & …, 2024 - aanda.org
Recent observations of volume-limited samples of magnetic white dwarfs (WD) have
revealed a higher incidence of magnetism in older stars. Specifically, these studies indicate …

Fluid mixing during phase separation in crystallizing white dwarfs

MH Montgomery, BH Dunlap - The Astrophysical Journal, 2024 - iopscience.iop.org
Accurate models of cooling white dwarfs must treat the energy released as their cores
crystallize. This phase transition slows the cooling by releasing latent heat and also …

A Short Intense Dynamo at the Onset of Crystallization in White Dwarfs

JR Fuentes, M Castro-Tapia… - The Astrophysical …, 2024 - iopscience.iop.org
The origin of large magnetic fields (≳ 10 6 G) in isolated white dwarfs is not clear. One
possible explanation is that crystallization of the star's core drives compositional convection …

Unveiling the white dwarf in J191213. 72− 441045.1 through ultraviolet observations

I Pelisoli, S Sahu, M Lyutikov, M Barkov… - Monthly Notices of …, 2024 - academic.oup.com
ABSTRACT J191213. 72− 441045.1 is a binary system composed of a white dwarf and an M-
dwarf in a 4.03-h orbit. It shows emission in radio, optical, and X-ray, all modulated at the …

Atmospheric heating and magnetism driven by 22Ne distillation in isolated white dwarfs

AF Lanza, NZ Rui, J Farihi, JD Landstreet… - Astronomy & …, 2024 - aanda.org
The origin of atmospheric heating in the cool, magnetic white dwarf GD 356 remains
unsolved nearly 40 years after its discovery. This once idiosyncratic star with T eff≈ 7500 K …