We present a set of full evolutionary sequences for white dwarfs with hydrogen-deficient atmospheres. We take into account the evolutionary history of the progenitor stars, all the relevant energy sources involved in the cooling, element diffusion in the very outer layers, and outer boundary conditions provided by new and detailed non-gray white dwarf model atmospheres for pure helium composition. These model atmospheres are based on the most up-to-date physical inputs. Our calculations extend down to very low effective temperatures, of ∼2500 K, provide a homogeneous set of evolutionary cooling tracks that are appropriate for mass and age determinations of old hydrogen-deficient white dwarfs, and represent a clear improvement over previous ...
We present a detailed calculation of model atmospheres for DA white dwarfs. Our atmosphere code solv...
White dwarf stars of spectral type DO populate the hot end of the hydrogen-deficient white dwarf coo...
We present evolutionary calculations and colors for massive white dwarfs with oxygen--neon cores f...
We present a set of full evolutionary sequences for white dwarfs with hydrogen-deficient atmospheres...
We present a set of full evolutionary sequences for white dwarfs with hydrogen-deficient atmospheres...
We present full evolutionary calculations appropriate for the study of hydrogen-rich DA white dwarfs...
We present full evolutionary calculations appropriate for the study of hydrogen-rich DA white dwarfs...
We present full evolutionary calculations appropriate for the study of hydrogen-rich DA white dwarfs...
We present full evolutionary calculations appropriate for the study of hot hydrogen-deficient DO whi...
We present full evolutionary calculations appropriate for the study of hot hydrogen-deficient DO whi...
We present full evolutionary calculations appropriate for the study of hot hydrogen-deficient DO whi...
We present full evolutionary calculations appropriate for the study of hot hydrogen-deficient DO whi...
We present full evolutionary calculations appropriate for the study of hot hydrogen-deficient DO whi...
We present detailed evolutionary calculations for carbon - oxygen - and helium - core white dwarf mo...
White dwarf stars of spectral type DO populate the hot end of the hydrogen-deficient white dwarf coo...
We present a detailed calculation of model atmospheres for DA white dwarfs. Our atmosphere code solv...
White dwarf stars of spectral type DO populate the hot end of the hydrogen-deficient white dwarf coo...
We present evolutionary calculations and colors for massive white dwarfs with oxygen--neon cores f...
We present a set of full evolutionary sequences for white dwarfs with hydrogen-deficient atmospheres...
We present a set of full evolutionary sequences for white dwarfs with hydrogen-deficient atmospheres...
We present full evolutionary calculations appropriate for the study of hydrogen-rich DA white dwarfs...
We present full evolutionary calculations appropriate for the study of hydrogen-rich DA white dwarfs...
We present full evolutionary calculations appropriate for the study of hydrogen-rich DA white dwarfs...
We present full evolutionary calculations appropriate for the study of hot hydrogen-deficient DO whi...
We present full evolutionary calculations appropriate for the study of hot hydrogen-deficient DO whi...
We present full evolutionary calculations appropriate for the study of hot hydrogen-deficient DO whi...
We present full evolutionary calculations appropriate for the study of hot hydrogen-deficient DO whi...
We present full evolutionary calculations appropriate for the study of hot hydrogen-deficient DO whi...
We present detailed evolutionary calculations for carbon - oxygen - and helium - core white dwarf mo...
White dwarf stars of spectral type DO populate the hot end of the hydrogen-deficient white dwarf coo...
We present a detailed calculation of model atmospheres for DA white dwarfs. Our atmosphere code solv...
White dwarf stars of spectral type DO populate the hot end of the hydrogen-deficient white dwarf coo...
We present evolutionary calculations and colors for massive white dwarfs with oxygen--neon cores f...