This is the final version. Available from Astronomical Society of the Pacific via the link in this recordEuroWD16: 20th European White Dwarf Workshop, 25-29 July 2016, Warwick, UKThe evolution of white dwarfs can be described as a cooling process. When the temperature is low enough, the interior experiences a phase transition and crystallizes. Crystallization introduces two new sources of energy, latent heat and chemical sedimentation, and induces the formation of a convective mantle around the solid core. This structure, which is analogous to that of the Earth, could induce the formation of a magnetic field via dynamo mechanism. In this work we discuss the viability of such mechanism, and its use as a diagnostic tool of crystallizatio...
The vast majority of stars that populate the Universe will end their evolution as white-dwarf stars....
We explore the physics of crystallization in the deep interiors of white dwarf (WD) stars using the ...
Despite thousands of spectroscopic detections, only four isolated white dwarfs exhibit Balmer emissi...
Isolated magnetic white dwarfs have field strengths ranging from kilogauss to gigagauss. However, th...
White dwarfs are stellar embers depleted of nuclear energy sources that cool over billions of years....
It has been recently suggested that white dwarfs generate magnetic fields in a process analogous to ...
The continuous cooling of a white dwarf is punctuated by events that affect its cooling rate. The mo...
We investigate whether the recently suggested rotation and crystallization driven dynamo can explain...
There are no known examples of magnetic white dwarfs with fields larger than ∼ 3 MG paired with a no...
We explore the physics of crystallization in the dense Coulomb plasma of the deep interiors of white...
We present the first radiation magnetohydrodynamic simulations of the atmosphere of white dwarf star...
The origin of strong (≳1MG) magnetic fields in white dwarfs has been a puzzle for decades. Recently,...
Abstract We investigate the luminosity suppression and its effect on the mass–radius ...
A significant fraction of white dwarfs harbour a magnetic field with strengths ranging from a few kG...
Using images from the Hubble Space Telescope Advanced Camera for Surveys, we measure the rate of coo...
The vast majority of stars that populate the Universe will end their evolution as white-dwarf stars....
We explore the physics of crystallization in the deep interiors of white dwarf (WD) stars using the ...
Despite thousands of spectroscopic detections, only four isolated white dwarfs exhibit Balmer emissi...
Isolated magnetic white dwarfs have field strengths ranging from kilogauss to gigagauss. However, th...
White dwarfs are stellar embers depleted of nuclear energy sources that cool over billions of years....
It has been recently suggested that white dwarfs generate magnetic fields in a process analogous to ...
The continuous cooling of a white dwarf is punctuated by events that affect its cooling rate. The mo...
We investigate whether the recently suggested rotation and crystallization driven dynamo can explain...
There are no known examples of magnetic white dwarfs with fields larger than ∼ 3 MG paired with a no...
We explore the physics of crystallization in the dense Coulomb plasma of the deep interiors of white...
We present the first radiation magnetohydrodynamic simulations of the atmosphere of white dwarf star...
The origin of strong (≳1MG) magnetic fields in white dwarfs has been a puzzle for decades. Recently,...
Abstract We investigate the luminosity suppression and its effect on the mass–radius ...
A significant fraction of white dwarfs harbour a magnetic field with strengths ranging from a few kG...
Using images from the Hubble Space Telescope Advanced Camera for Surveys, we measure the rate of coo...
The vast majority of stars that populate the Universe will end their evolution as white-dwarf stars....
We explore the physics of crystallization in the deep interiors of white dwarf (WD) stars using the ...
Despite thousands of spectroscopic detections, only four isolated white dwarfs exhibit Balmer emissi...