No nearby counterparts to the moving objects in the Hubble Deep Field
arXiv:astro-ph/9912264 · doi:10.1046/j.1365-8711.2001.04082.x
Abstract
Ibata et al (1999) have recently discovered faint, moving objects in the Hubble Deep Field. The quantity, magnitudes and proper motions of these objects are consistent with old white dwarfs making up the Galactic dark halo. We review a number of ground-based proper motion surveys in which nearby dark halo white dwarfs might be present, if they have the colours and absolute magnitudes proposed. No such objects have been found, whereas we argue here that several times more would be expected than in the Hubble Deep Field. We conclude it is unlikely that hydrogen atmosphere white dwarfs make up a significant fraction of the halo dark matter. No limits can be placed yet on helium atmosphere dwarfs from optical searches.
arXiv comment7 pages, 4 figures, MNRAS LaTeX format
References in corpus (16)
- The MACHO Project: Microlensing Results from 5.7 Years of LMC Observations
- Cooling Models for Old White Dwarfs
- A Survey for Cool White Dwarfs and the age of the Galactic Disc
- Is Galactic Dark Matter White ?
- A Very Low-Luminosity, Very Cool, DC White Dwarf
- Faint, moving objects in the Hubble Deep Field: components of the dark halo?
- Isochrones and Luminosity Functions for Old White Dwarfs
- A Survey for Faint Stars of Large Proper Motion Using Extra Poss II Plates
- Nearby Microlensing Events - Identification of the Candidates for the SIM
- Massive Compact Halo Objects Viewed from a Cosmological Perspective: Contribution to the Baryonic Mass Density of the Universe
- Post-Newtonian Theory for Precision Doppler Measurements of Binary Star Orbits
- Quasar Candidates in the Hubble Deep Field
- Vacuum Breakdown near a Black Hole Charged by Hypercritical Accretion
- MACHOs, White Dwarfs, and the Age of the Universe
- Constraining the cosmic abundance of stellar remnants with multi-TeV gamma-rays
- The Origin of Primordial Dwarf Stars and Baryonic Dark Matter
Cited by in corpus (19)
- A Catalog of Northern Stars With Annual Proper Motions Larger Than 0.15 Seconds of Arc (LSPM catalog - North)
- Direct Detection of Galactic Halo Dark Matter
- A Determination of the Local Density of White Dwarf Stars
- Meeting the Cool Neighbours I: Nearby stars in the NLTT Catalogue - Defining the sample
- High-velocity white dwarfs: thick disk, not dark matter
- Monte Carlo simulations of the halo white dwarf population
- The Liverpool-Edinburgh High Proper Motion Survey
- The white dwarf luminosity function
- Improved Astrometry and Photometry for the Luyten Catalog. I. Bright Stars
- LSR0602+3910 - Discovery of a Bright Nearby L-type Brown Dwarf
- The Galactic Inner Halo: Searching for White Dwarfs and Measuring the Fundamental Galactic Constant, Vo/Ro
- White dwarfs and Galactic dark matter
- EROS 2 proper motion survey: Constraints on the halo white dwarfs
- Absolute Proper Motions to B~22.5: IV. Faint, Low Velocity White Dwarfs and the White Dwarf Population Density Law
- Completeness of USNO-B for High Proper-Motion Stars
- Simulating a White Dwarf-dominated Galactic Halo
- The Galactic Halo from Microlensing
- Dark halo baryons not in ancient halo white dwarfs
- White dwarfs with hydrogen-deficient atmospheres and the dark matter content of the Galaxy