Volume 378, Number 3, November II 2001
|Page(s)||L53 - L56|
|Published online||15 November 2001|
On high proper motion white dwarfs from photographic surveys
CNRS UMR6091, Observatoire de Besançon, BP1615, 25010 Besançon Cedex, France
2 Université de Bretagne-Sud, BP 573, 56017 Vannes Cedex, France
Corresponding author: C. Reylé, email@example.com
Accepted: 15 September 2001
The interpretation of high proper motion white dwarfs detected by Oppenheimer et al. ([CITE]) was the start of a lively controversy. While the discoverers identify a large fraction of their findings as dark halo members, others interpret the same sample as essentially made of disc and/or thick disc stars. We use the comprehensive description of Galactic stellar populations provided by the "Besançon" model to produce a realistic simulation of Oppenheimer et al. data, including all observational selections and calibration biases. The conclusion is unambiguous: Thick disc white dwarfs resulting from ordinary hypotheses on the local density and kinematics are sufficient to explain the observed objects, there is no need for halo white dwarfs. This conclusion is robust to reasonable changes in model ingredients. The main cause of the misinterpretation seems to be that the velocity distribution of a proper motion selected star sample is severely biased in favour of high velocities. This has been neglected in previous analyses. Obviously this does not prove that no such objects like halo white dwarfs can exist, but Oppenheimer et al. observations drive their possible contribution in the dark matter halo down to an extremely low fraction.
Key words: cosmology: dark matter / Galaxy: structure / Galaxy: stellar content / Galaxy: general
© ESO, 2001
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.