Add to ORKGWhite dwarf cooling theory and very deep observations in star clusters provide a new tool to test stellar evolution theory and time scales. In particular, white dwarf cooling theory is now testing the degree of enhanced core mixing in stars with turnoff ages of 1 to 2 Gyr. More generally, I show the good overall agreement between white dwarf and modern isochrone ages over the range 0.1 to 4 Gyr
textOur group has developed a Bayesian modeling technique to determine the ages of stellar populatio...
textOur group has developed a Bayesian modeling technique to determine the ages of stellar populatio...
The white dwarf luminosity function of a stellar cluster will have a sharp trunca- tion at a luminos...
White dwarf cooling theory and very deep observations in star clusters provide a new tool to test st...
I explore the current ability of both white dwarf cooling theory and main sequence stellar evolution...
ABSTRACT I explore the current ability of both white dwarf cooling theory and main sequence stellar ...
textOpen clusters have long been objects of interest in astronomy. As a good approximation of essen...
textOpen clusters have long been objects of interest in astronomy. As a good approximation of essen...
I explore the current ability of both white dwarf cooling theory and main-sequence stellar evolution...
Context. Within the theoretical framework of some modern unification theories the constants of natur...
White dwarfs are the most common stellar evolutionary end-point. Moreover, they can be considered as...
White dwarfs are the most common stellar evolutionary end-point. Moreover, they can be considered as...
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...
ABSTRACT. In the light of recent significant progress on both the observational and theoretical fron...
textOur group has developed a Bayesian modeling technique to determine the ages of stellar populatio...
textOur group has developed a Bayesian modeling technique to determine the ages of stellar populatio...
The white dwarf luminosity function of a stellar cluster will have a sharp trunca- tion at a luminos...
White dwarf cooling theory and very deep observations in star clusters provide a new tool to test st...
I explore the current ability of both white dwarf cooling theory and main sequence stellar evolution...
ABSTRACT I explore the current ability of both white dwarf cooling theory and main sequence stellar ...
textOpen clusters have long been objects of interest in astronomy. As a good approximation of essen...
textOpen clusters have long been objects of interest in astronomy. As a good approximation of essen...
I explore the current ability of both white dwarf cooling theory and main-sequence stellar evolution...
Context. Within the theoretical framework of some modern unification theories the constants of natur...
White dwarfs are the most common stellar evolutionary end-point. Moreover, they can be considered as...
White dwarfs are the most common stellar evolutionary end-point. Moreover, they can be considered as...
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...
ABSTRACT. In the light of recent significant progress on both the observational and theoretical fron...
textOur group has developed a Bayesian modeling technique to determine the ages of stellar populatio...
textOur group has developed a Bayesian modeling technique to determine the ages of stellar populatio...
The white dwarf luminosity function of a stellar cluster will have a sharp trunca- tion at a luminos...