SIMBAD references

2012A&A...546L...3C - Astronomy and Astrophysics, volume 546L3-3 (2012/10-1)

The brightest pure-H ultracool white dwarf.

CATALAN S., TREMBLAY P.-E., PINFIELD D.J., SMITH L.C., ZHANG Z.H., NAPIWOTZKI R., MAROCCO F., DAY-JONES A.C., GOMES J., FORDE K.P., LUCAS P.W. and JONES H.R.A.

Abstract (from CDS):

We report the identification of LSR J0745+2627 in the United Kingdom InfraRed Telescope Infrared Deep Sky Survey (UKIDSS) Large Area Survey (LAS) as a cool white dwarf with kinematics and age compatible with the thick-disk/halo population. LSR J0745+2627 has a high proper motion (890mas/yr) and a high reduced proper motion value in the J band (HJ=21.87). We show how the infrared-reduced proper motion diagram is useful for selecting a sample of cool white dwarfs with low contamination. LSR J0745+2627 is also detected in the Sloan Digital Sky Survey (SDSS) and the Wide-field Infrared Survey Explorer (WISE). We have spectroscopically confirmed this object as a cool white dwarf using X-Shooter on the Very Large Telescope. A detailed analysis of its spectral energy distribution reveals that its atmosphere is compatible with a pure-H composition model with an effective temperature of 3880±90K. This object is the brightest pure-H ultracool white dwarf (Teff<4000K) ever identified. We have constrained the distance (24-45pc), space velocities and age considering different surface gravities. The results obtained suggest that LSR J0745+2627 belongs to the thick-disk/halo population and is also one of the closest ultracool white dwarfs.

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Journal keyword(s): white dwarfs - stars: Population II - stars: abundances - stars: individual: ULAS J074509.02+262705.0 - stars: individual: SDSS J074509.02+262705.0 - stars: fundamental parameters

VizieR on-line data: <Available at CDS (J/A+A/546/L3): table.dat>

Simbad objects: 8

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