Abstract
We present a model of the solar neighbourhood (d<100 pc) white dwarf (WD) population and show its distribution in e®ective temperature and mass. The WDs are created by the death-rate of a population model matching the local stars observed by hipparcos, considering depletion as caused by the \thin disk" dynamics.
| Original language | English |
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| Title of host publication | In: Procs of the 14th European Workshop on White Dwarfs - ASP Conference Series 334 |
| Publisher | Astronomical Society of the Pacific |
| Pages | 93-98 |
| ISBN (Print) | 1-58381-197-4, 978-1-58381-268-6 |
| Publication status | Published - 2005 |