Add to ORKGThe Sloan Digital Sky Survey has allowed us to increase the number of known white dwarfs by a factor of five and consequently the number of known pulsating white dwarfs also by a factor of five. It has also led to the discovery of new types of variable white dwarfs, as the variable hot DQs, and the pulsating Extremely Low Mass white dwarfs. With the Kepler Mission, it has been possible to discover new phenomena, the outbursts present in a few pulsating white dwarfs
White dwarfs represent the end point of stellar evolution for the majority of stars. As such, they a...
We identify seven new ultracool white dwarfs discovered in the Sloan Digital Sky Survey (SDSS). The ...
Accreting white dwarfs have recently been shown to exhibit non-radial pulsations similar to their no...
The Sloan Digital Sky Survey has allowed us to increase the number of known white dwarfs by a factor...
The Sloan Digital Sky Survey has allowed us to increase the number of known white dwarfs by a factor...
The Sloan Digital Sky Survey has allowed us to increase the number of known white dwarfs by a factor...
The number of discovered non-radially pulsating white dwarfs (WDs) in cataclysmic variables (CVs) is...
We are searching for new He atmosphere white dwarf pulsators (DBVs) based on the newly found white d...
We are searching for new He atmosphere white dwarf pulsators (DBVs) based on the newly found white d...
We present 35 new pulsating DA (hydrogen atmosphere) white dwarf stars discovered from the Sloan Dig...
We present 35 new pulsating DA (hydrogen atmosphere) white dwarf stars discovered from the Sloan Dig...
We present 35 new pulsating DA (hydrogen atmosphere) white dwarf stars discovered from the Sloan Dig...
We present 35 new pulsating DA (hydrogen atmosphere) white dwarf stars discovered from the Sloan Dig...
The discovery in 1998 of a pulsating white dwarf in the cataclysmic variable GW Lib opened up a new ...
We report the discovery of five very cool white dwarfs in the Sloan Digital Sky Survey (SDSS). Four ...
White dwarfs represent the end point of stellar evolution for the majority of stars. As such, they a...
We identify seven new ultracool white dwarfs discovered in the Sloan Digital Sky Survey (SDSS). The ...
Accreting white dwarfs have recently been shown to exhibit non-radial pulsations similar to their no...
The Sloan Digital Sky Survey has allowed us to increase the number of known white dwarfs by a factor...
The Sloan Digital Sky Survey has allowed us to increase the number of known white dwarfs by a factor...
The Sloan Digital Sky Survey has allowed us to increase the number of known white dwarfs by a factor...
The number of discovered non-radially pulsating white dwarfs (WDs) in cataclysmic variables (CVs) is...
We are searching for new He atmosphere white dwarf pulsators (DBVs) based on the newly found white d...
We are searching for new He atmosphere white dwarf pulsators (DBVs) based on the newly found white d...
We present 35 new pulsating DA (hydrogen atmosphere) white dwarf stars discovered from the Sloan Dig...
We present 35 new pulsating DA (hydrogen atmosphere) white dwarf stars discovered from the Sloan Dig...
We present 35 new pulsating DA (hydrogen atmosphere) white dwarf stars discovered from the Sloan Dig...
We present 35 new pulsating DA (hydrogen atmosphere) white dwarf stars discovered from the Sloan Dig...
The discovery in 1998 of a pulsating white dwarf in the cataclysmic variable GW Lib opened up a new ...
We report the discovery of five very cool white dwarfs in the Sloan Digital Sky Survey (SDSS). Four ...
White dwarfs represent the end point of stellar evolution for the majority of stars. As such, they a...
We identify seven new ultracool white dwarfs discovered in the Sloan Digital Sky Survey (SDSS). The ...
Accreting white dwarfs have recently been shown to exhibit non-radial pulsations similar to their no...