2014ApJ...788..103T


Query : 2014ApJ...788..103T

2014ApJ...788..103T - Astrophys. J., 788, 103 (2014/June-3)

White dwarfs in the UKIRT infrared deep sky survey data release 9.

TREMBLAY P.-E., LEGGETT S.K., LODIEU N., FREYTAG B., BERGERON P., KALIRAI J.S. and LUDWIG H.-G.

Abstract (from CDS):

We have identified 8 to 10 new cool white dwarfs from the Large Area Survey (LAS) Data Release 9 of the United Kingdom InfraRed Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS). The data set was paired with the Sloan Digital Sky Survey to obtain proper motions and a broad ugrizYJHK wavelength coverage. Optical spectroscopic observations were secured at Gemini Observatory and confirm the degenerate status for eight of our targets. The final sample includes two additional white dwarf candidates with no spectroscopic observations. We rely on improved one-dimensional model atmospheres and new multi-dimensional simulations with CO5BOLD to review the stellar parameters of the published LAS white dwarf sample along with our additional discoveries. Most of the new objects possess very cool atmospheres with effective temperatures below 5000 K, including two pure-hydrogen remnants with a cooling age between 8.5 and 9.0 Gyr, and tangential velocities in the range 40 km/s ≤ vtan ≤ 60 km/s. They are likely thick disk 10-11 Gyr old objects. In addition, we find a resolved double degenerate system with vtan∼ 155 km/s and a cooling age between 3.0 and 5.0 Gyr. These white dwarfs could be disk remnants with a very high velocity or former halo G stars. We also compare the LAS sample with earlier studies of very cool degenerates and observe a similar deficit of helium-dominated atmospheres in the range 5000 < Teff(K) < 6000. We review the possible explanations for the spectral evolution from helium-dominated toward hydrogen-rich atmospheres at low temperatures.

Abstract Copyright: ∼

Journal keyword(s): infrared: stars - stars: fundamental parameters - surveys - techniques: photometric - techniques: spectroscopic - white dwarfs

CDS comments: ULAS sources not in Table 1 are not identified.

Simbad objects: 21

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Number of rows : 21
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SDSS J002439.96-003039.6 WD* 00 24 39.9649960656 -00 30 39.288617784           DC 6 0
2 ULAS J010041.25+110329.5 * 01 00 41.2563012048 +11 03 29.476497384           ~ 1 0
3 SDSS J011355.25-025729.9 * 01 13 55.2491253408 -02 57 29.930067972           ~ 1 0
4 SDSS J013021.48-044105.9 QSO 01 30 21.4776706224 -04 41 05.978699700           ~ 8 0
5 ULAS J015609.77-001450.3 NIR 01 56 09.773 -00 14 50.40           ~ 1 0
6 ULAS J034933.39-002111.1 NIR 03 49 33.444 -00 21 10.70           ~ 1 0
7 ULAS J081553.52+242734.7 WD? 08 15 53.4612788256 +24 27 35.298873828           ~ 4 0
8 ULAS J083836.19+240305.8 NIR 08 38 36.2006565672 +24 03 05.673518028           ~ 1 0
9 ULAS J091656.77+304727.2 NIR 09 16 56.7760025016 +30 47 27.101696712           ~ 1 0
10 LSPM J1240+2559B WD? 12 40 29.3521067472 +25 59 48.295334004           ~ 5 0
11 LSPM J1240+2559A WD* 12 40 29.5638288504 +25 59 47.826564144           DA 6 0
12 LSPM J1247+0646 WD* 12 47 39.1272104568 +06 46 04.304355463   20.2   18.5   DQpec 23 1
13 LSPM J1409+0743 WD* 14 09 44.2963739640 +07 43 55.135265340   20.0   18.9   DA: 9 0
14 LSPM J1607+2608 WD* 16 07 38.9462962032 +26 08 46.685376600   21.2   19.0   DA: 9 0
15 ULAS J164026.38+281152.3 NIR 16 40 26.3893631136 +28 11 52.183653000           ~ 1 0
16 SDSS J215300.68+452733.2 * 21 53 00.6733864032 +45 27 33.288824268           ~ 1 0
17 SDSS J220623.89+022447.2 WD? 22 06 23.8734455856 +02 24 47.773955988           ~ 6 0
18 LSPM J2242+0048 WD* 22 42 06.1779800472 +00 48 22.931536572   20.1   18.7   DC 21 0
19 ULAS J231554.62-001332.6 NIR 23 15 54.6226096128 -00 13 32.964018132           ~ 1 0
20 ULAS J233022.56+054022.1 WD* 23 30 22.4939846184 +05 40 23.459873880           DA: 6 0
21 ULAS J233147.27-004906.4 WD* 23 31 47.273 -00 49 06.48           DA 2 0

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