The Ages of Very Cool Hydrogen-rich White Dwarfs

@article{Salaris2000TheAO,
  title={The Ages of Very Cool Hydrogen-rich White Dwarfs},
  author={Maurizio Salaris and Enrique Garc{\'i}a-Berro and M L Hernanz and Jordi Isern and D. M. Neumann Liverpool Jmu and Upc Barcelona and Ieec Barcelona and Vanderbilt University},
  journal={The Astrophysical Journal},
  year={2000},
  volume={544},
  pages={1036-1043}
}
The evolution of white dwarfs is essentially a cooling process that depends primarily on the energy stored in their degenerate cores and on the transparency of their envelopes. In this paper we compute accurate cooling sequences for carbon-oxygen white dwarfs with hydrogen dominated atmospheres for the full range of masses of interest. For this purpose we use the most accurate available physical inputs for both the equation of state and opacities of the envelope and for the thermodynamic… 

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