Add to ORKGWe demonstrate that the peculiar line profiles observed in DA white dwarfs in the temperature range of the ZZ Ceti variables can be explained by the surface velocity fields associated with the pulsations
We present the first asteroseismological study for 42 massive ZZ Ceti stars based on a large set of ...
Context. ZZ Ceti stars are pulsating white dwarfs with a carbon-oxygen core build up during the core...
The mean pulsation period of ZZ Ceti stars increases with decreasing effective temperature as we tra...
The location of the red edge of the ZZ Ceti instability strip is defined observationally as being th...
ZZ Ceti stars form the most numerous group of degenerate variable stars. They are otherwise normal D...
The sharp Hα NLTE line cores of hydrogen-rich (DA) white dwarfs allow their projected rotational vel...
We compute new chemical profiles for the core and envelope of white dwarfs appropriate for pulsation...
We calculate an extensive adiabatic model grid for pulsating white dwarfs with H dominated atmospher...
Numerical simulations of light curves of variable DA white dwarfs (ZZ Ceti stars) predict flux ampli...
The current status of theoretical understanding of the oscillations observed in the ZZ Ceti stars an...
We present time-resolved spectrophotometry of the pulsating DA white dwarf G29-38. As in previous br...
We perform ground-based photometric observations of 22 DA white dwarf stars, 10 already known ZZ Cet...
We present photometry and spectroscopy for 27 pulsating hydrogen-atmosphere white dwarfs (DAVs; a.k....
We present time-resolved spectrophotometry of the pulsating DA white dwarf G 29-38. As in previous b...
We present a detailed analysis of time-resolved optical spectra of the ZZ Ceti white dwarf, HS 0507+...
We present the first asteroseismological study for 42 massive ZZ Ceti stars based on a large set of ...
Context. ZZ Ceti stars are pulsating white dwarfs with a carbon-oxygen core build up during the core...
The mean pulsation period of ZZ Ceti stars increases with decreasing effective temperature as we tra...
The location of the red edge of the ZZ Ceti instability strip is defined observationally as being th...
ZZ Ceti stars form the most numerous group of degenerate variable stars. They are otherwise normal D...
The sharp Hα NLTE line cores of hydrogen-rich (DA) white dwarfs allow their projected rotational vel...
We compute new chemical profiles for the core and envelope of white dwarfs appropriate for pulsation...
We calculate an extensive adiabatic model grid for pulsating white dwarfs with H dominated atmospher...
Numerical simulations of light curves of variable DA white dwarfs (ZZ Ceti stars) predict flux ampli...
The current status of theoretical understanding of the oscillations observed in the ZZ Ceti stars an...
We present time-resolved spectrophotometry of the pulsating DA white dwarf G29-38. As in previous br...
We perform ground-based photometric observations of 22 DA white dwarf stars, 10 already known ZZ Cet...
We present photometry and spectroscopy for 27 pulsating hydrogen-atmosphere white dwarfs (DAVs; a.k....
We present time-resolved spectrophotometry of the pulsating DA white dwarf G 29-38. As in previous b...
We present a detailed analysis of time-resolved optical spectra of the ZZ Ceti white dwarf, HS 0507+...
We present the first asteroseismological study for 42 massive ZZ Ceti stars based on a large set of ...
Context. ZZ Ceti stars are pulsating white dwarfs with a carbon-oxygen core build up during the core...
The mean pulsation period of ZZ Ceti stars increases with decreasing effective temperature as we tra...