Abstract
We report the discovery of an ultra-cool white dwarf in the COMBO-17 survey. So far, only seven objects have been discovered in this rare category of white dwarfs, which are characterized by strong flux depression in the far-red and near-infrared part of the spectrum, presumably due to collisionally induced absorption (CIA). The new object COMBO-17 J114356.08-0144032 has very similar colours to LHS 3250, which was the first of its kind to be recognized. However, at R = 21.5 it is the faintest and possibly most distant such object discovered to date. It is the only such object in COMBO-17 at R < 23; due to the small sky coverage of 0.78 □ this chance discovery can not provide any constraints on the abundance of faint ultra-cool white dwarfs. We speculate on the basis of the proper motion that this new object is probably a member of the Galactic (thin) disk.
| Original language | English |
|---|---|
| Pages (from-to) | L49-L52 |
| Journal | Astronomy and Astrophysics |
| Volume | 444 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - Dec 2005 |
| Externally published | Yes |
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