Dark halo baryons not in ancient halo white dwarfs
arXiv:astro-ph/0403543 · doi:10.1051/0004-6361:20040491
Abstract
Having ruled out the possibility that stellar objects are the main contributor of the dark matter embedding galaxies, microlensing experiments cannot exclude the hypothesis that a significant fraction of the Milky Way dark halo might be made of MACHOs with masses in the range $0.5-0.8 \msun$. Ancient white dwarfs are generally considered the most plausible candidates for such MACHOs. We report the results of a search for such white dwarfs in a proper motion survey covering a 0.16 sqd field at three epochs at high galactic latitude, and 0.938 sqd at two epochs at intermediate galactic latitude (VIRMOS survey), using the CFH telescope. Both surveys are complete to I = 23, with detection efficiency fading to 0 at I = 24.2. Proper motion data are suitable to separate unambiguously halo white dwarfs identified by belonging to a non rotating system. No candidates were found within the colour-magnitude-proper motion volume where such objects can be safely discriminated from any standard population as well as from possible artefacts. In the same volume, we estimate the maximum white dwarf halo fraction compatible with this observation at different significance levels if the halo is at least 14 gigayears old and under different ad hoc initial mass functions. Our data alone rules out a halo fraction greater than 14% at 95% confidence level. Combined with two previous investigations exploring comparable volumes pushes the limit below 4 % (95% confidence level) or below 1.3% (64% confidence), this implies that if baryonic dark matter is present in galaxy halos, it is not, or it is only marginally in the form of faint hydrogen white dwarfs.
accepted in Astronomy and Astrophysics (19-05-2004)
References in corpus (19)
- Evolutionary models for very-low-mass stars and brown dwarfs with dusty atmospheres
- The MACHO Project LMC Microlensing Results from the First Two Years and the Nature of the Galactic Dark Halo
- Direct Detection of Galactic Halo Dark Matter
- The VIRMOS deep imaging survey II: CFH12K BVRI optical data for the 0226-04 deep field
- Pure hydrogen atmosphere for very cool white dwarfs
- The VIRMOS deep imaging survey: I. overview and survey strategy
- Cooling sequences and color-magnitude diagrams for cool white dwarfs with hydrogen-atmospheres
- Discovery of high proper motion ancient white dwarfs: nearby massive compact halo objects?
- High-velocity white dwarfs: thick disk, not dark matter
- Is Galactic Dark Matter White ?
- High proper motion white dwarfs and halo dark matter
- Faint, moving objects in the Hubble Deep Field: components of the dark halo?
- On high proper motion white dwarfs from photographic surveys
- No nearby counterparts to the moving objects in the Hubble Deep Field
- White dwarfs and Galactic dark matter
- A Proper Motion Survey for White Dwarfs with the Wide Field Planetary Camera 2
- EROS 2 proper motion survey: Constraints on the halo white dwarfs
- Illuminating the darkness: More evidence from faint-star proper-motions for a cool and warm component to the local dark matter in the Galaxy
- Simulating a White Dwarf-dominated Galactic Halo
Cited by in corpus (6)
- Testing LMC Microlensing Scenarios: The Discrimination Power of the SuperMACHO Microlensing Survey
- Stellar populations in the CFHTLS. I. New constraints on the IMF at low mass
- Trigonometric parallaxes of high velocity halo white dwarf candidates
- Galaxy Formation and Dark Matter
- Searching for Gravitational Radiation from Binary Black Hole MACHOs in the Galactic Halo
- Astrophysics in 2005