Summary. During the last decade white dwarfs have become important as tools in many areas beyond traditional stellar physics: from the age determination of the stars in the solar neighborhood to the dating of open clusters and the distance determina-tion of globular clusters. They are primary candidates for the MACHO microlensing events, possibly for a stellar component of the dark halo, and for the supernova Ia progenitors. The recent developments in these areas are reviewed, but some highlights from more “mature ” areas such as stellar parameters, mass distributions, magnetic, and pulsating white dwarfs are also summarized briefly
White dwarfs are the final remnants of low- and intermediate-mass stars. Their evolution is essentia...
We describe a new survey for cool white dwarfs that supplements Sloan Digital Sky Survey photometry ...
Abstract: The development of far-UV astronomy has been particularly important for the study of hot w...
We present a brief summary of what is currently known about white dwarf stars, with an emphasis on t...
We present a brief summary of what is currently known about white dwarf stars, with an emphasis on t...
We present a brief summary of what is currently known about white dwarf stars, with an emphasis on t...
We present a brief summary of what is currently known about white dwarf stars, with an emphasis on t...
In this review I describe the basic properties of white dwarfs and their pulsations. I then discuss ...
In this review I describe the basic properties of white dwarfs and their pulsations. I then discuss ...
Every two years, white dwarf researchers and enthusiasts meet to exchange their knowledge and discus...
ABSTRACT. In the light of recent significant progress on both the observational and theoretical fron...
White dwarfs are a class of stars with unique physical properties. They present many challenging pro...
The discovery in 1998 of a pulsating white dwarf in the cataclysmic variable GW Lib opened up a new ...
The vast majority of stars that populate the Universe will end their evolution as white-dwarf stars....
White dwarfs are the end products of the entire stellar evolutionary process in all intermediate an...
White dwarfs are the final remnants of low- and intermediate-mass stars. Their evolution is essentia...
We describe a new survey for cool white dwarfs that supplements Sloan Digital Sky Survey photometry ...
Abstract: The development of far-UV astronomy has been particularly important for the study of hot w...
We present a brief summary of what is currently known about white dwarf stars, with an emphasis on t...
We present a brief summary of what is currently known about white dwarf stars, with an emphasis on t...
We present a brief summary of what is currently known about white dwarf stars, with an emphasis on t...
We present a brief summary of what is currently known about white dwarf stars, with an emphasis on t...
In this review I describe the basic properties of white dwarfs and their pulsations. I then discuss ...
In this review I describe the basic properties of white dwarfs and their pulsations. I then discuss ...
Every two years, white dwarf researchers and enthusiasts meet to exchange their knowledge and discus...
ABSTRACT. In the light of recent significant progress on both the observational and theoretical fron...
White dwarfs are a class of stars with unique physical properties. They present many challenging pro...
The discovery in 1998 of a pulsating white dwarf in the cataclysmic variable GW Lib opened up a new ...
The vast majority of stars that populate the Universe will end their evolution as white-dwarf stars....
White dwarfs are the end products of the entire stellar evolutionary process in all intermediate an...
White dwarfs are the final remnants of low- and intermediate-mass stars. Their evolution is essentia...
We describe a new survey for cool white dwarfs that supplements Sloan Digital Sky Survey photometry ...
Abstract: The development of far-UV astronomy has been particularly important for the study of hot w...