Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-09-15
Astronomy and Astrophysics
Astrophysics
18 pages, 14 postscript figures. Accepted for publication in Monthly Notices of the RAS, uses mn.sty
Scientific paper
In order to understand the dynamical and chemical evolution of our Galaxy it is of fundamental importance to study the local neighborhood. White dwarf stars are ideal candidates to probe the history of the solar neighborhood, since these ``fossil'' stars have very long evolutionary time-scales and, at the same time, their evolution is relatively well understood. In fact, the white dwarf luminosity function has been used for this purpose by several authors. However, a long standing problem arises from the relatively poor statistics of the samples, especially at low luminosities. In this paper we assess the statistical reliability of the white dwarf luminosity function by using a Monte Carlo approach.
Burkert Andreas
Garcia-Berro Enrique
Isern Jordi
Torres Santiago
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