Titlebook: White Dwarfs; Proceedings of the 9 Detlev Koester,Klaus Werner Conference proceedings 1995 Springer-Verlag Berlin Heidelberg 1995 Anomalie.

modest

0075-8450 e the most important events in this field. Many of the contributions, however, have been expanded considerably by the authors to include introductory material. This makes this volume a useful, up-to-date introduction into the present status of observations and theory of white dwarf stars.978-3-662-1

NATTY

Theoretical white dwarf luminosity functions: DA models, is in the range 6.5 to 11 Gyr. Phase separation of crystallizing C/O-core models has the potential to add up to ～20% to the ages of the coolest WDs, but the suggested process by which the matter is redistributed in the core is not sufficiently compelling.

Excise

Nmda-Receptor

What is wrong with stellar modeling, stellar modeling will be provided, in the attempt of convincing the reader that, switching from local stellar models to non-local, turbulent ones, will be a major, generational leap, which will greatly extend the boundaries of our quantitative understanding of stellar evolution

textile

Thirty years of white dwarf research in retrospect,He-rich white dwarfs with metal lines (spectral type DZ), the evaluation of color-color and color-magnitude diagrams, the determination of masses and the mass distribution for H-rich stars (spectral type DA), and the derivation of initial-to-final mass relations for stellar and galactic evolution.

ANTH

針葉

談判

What is wrong with stellar modeling,onably good . understanding of what is going on in the vast majority of the cases, and we also quantitatively know many details on simple stellar structures (even if the solar neutrino problem is always a warning to be frequently reminded). In the following, a short review of the basic problems with

Foolproof

FOR

Conference proceedings 1995 important events in this field. Many of the contributions, however, have been expanded considerably by the authors to include introductory material. This makes this volume a useful, up-to-date introduction into the present status of observations and theory of white dwarf stars.