White Dwarfs Proceedings of the 10th European Workshop on White Dwarfs, held in Blanes, Spain, 17–21 June 1996

The study of white dwarfs has been steadily growing during the last years and now is a mature field extending its influence over many others. Since white dwarfs are long lived objects, they can be used to obtain information about the history of the Galaxy. The simplicity of their structures enables...

Full description

Corporate Author: SpringerLink (Online service)
Other Authors: Isern, J. (Editor), Hernanz, M. (Editor), García-Berro, E. (Editor)
Format: eBook
Language:English
Published: Dordrecht Springer Netherlands 1997, 1997
Edition:1st ed. 1997
Series:Astrophysics and Space Science Library
Subjects:
Online Access:
Collection: Springer Book Archives -2004 - Collection details see MPG.ReNa
Table of Contents:
  • first results
  • Preliminary asteroseismology of G 29–38
  • Recent advances in the theoretical determination of the ZZ Ceti instability strip
  • Cool DAV asteroseismology
  • Overstability of g-modes in ZZ Ceti variables
  • A continuing spectroscopic study of the instability strip of the pulsating DB (V 777 Her) white dwarfs: the view in the optical
  • The potential of asteroseismology for hot, B subdwarfs: a new class of pulsating stars?
  • Modeling time-resolved spectra of ZZ Ceti stars
  • Discovery of two new ZZ Ceti variables
  • Non-pulsating DA white dwarfs in the DAV region
  • CO white dwarfs near the Chandrasekhar limiting mass
  • The Accretion-Induced Collapse of white dwarfs revisited in 3D
  • II. Luminosity Functions and Populations
  • Towards a luminosity function of hot DA white dwarfs
  • New results on PG 1159 stars and ultrahigh-excitation DO white dwarfs
  • Non-LTE analyses of DO white dwarfs
  • New spectral analyses of pre-white dwarfs
  • The sphericity effects in the NLTE model atmospheres of white dwarfs
  • Heavy elements in white dwarf envelopes
  • Lyman spectra of hot DA white dwarfs
  • Diffusion of silicon in the envelopes of hot DA white dwarfs
  • Time-dependent diffusion calculations for hot pre-white dwarfs
  • Evolutionary calculations of carbon dredge-up in helium envelope white dwarfs
  • Analysis of optical and ultraviolet spectroscopy of the DAZ white dwarf G 74–7
  • Modeling extreme ultraviolet spectra of white dwarfs with high-metallicity LTE models
  • Extreme ultraviolet spectroscopy of EUVE J0720-317 and EUVE J0723-277
  • A new dithered EUVE spectrum of PG 1234+482
  • Line of sight H and He ionization fractions in the local interstellar medium
  • An instrument for observations of EUV opacity sources in G 191-B2B
  • a new infrared search
  • The EC 14026 stars: a new class of pulsating star
  • Hot white dwarfs in non-interacting binaries from the ROSAT EUV survey
  • HST observations of AM Canum Venaticorum
  • Effects of irradiation on the secondary star in a tight binary system, exemplified by AM Canum Venaticorum
  • White dwarfs in AM Herculis systems
  • HST synthetic spectral analysis of U Gem in early and late quiescence: a heated white dwarf and accretion belt
  • WFPC2 observations of Procyon B
  • Extreme ultraviolet light curve and phase-resolved spectroscopy of the hot white dwarf in V 471 Tauri
  • Unique white dwarfs accompanying recycled pulsars
  • Merging of different mass ratio white dwarfs: first moments of the 0.4–1.2 M? case
  • V. Magnetic White Dwarfs
  • a conservative point of view
  • Halo white dwarfs: a non conventional scenario
  • HST observations of white dwarfs in the globular cluster NGC 6397
  • The distance and age of the globular cluster NGC 6752 measured by HST observations of cluster and field white dwarfs
  • DA white dwarfs in the Montréal-Cambridge-Tololo survey
  • Cool white dwarf survey using stacked digitised Schmidt plates
  • III. Atmospheres
  • Chemical evolution of cool white dwarf’s atmospheres
  • The chemical evolution of white dwarf stars: what the observations tell us
  • A critical look at the question of thick vs thin hydrogen and helium envelopes in white dwarfs
  • Polyatomic carbon molecules in very cool helium-rich white dwarfs
  • Analysis of optical, UV and EUV observations of G 191-B2B