All names: SDSS J105133.36+663401.1, SDSS J105133.35+663400.9, TIC 142808656, WD 1048+668, SDSS J105133.36+663400.7, SDSS J105133.35+663401.0, GALEX J105133.2+663401, 2MASS J10513336+6634012, SDSS J105133.34+663401.0, WIRED J105133.35+663401.0, SDSS J105133.36+663401.3, Gaia DR3 1059664849644881152, [HHD2009] SDSS J1051+6634, Gaia EDR3 1059664849644881152, Gaia DR2 1059664849644881152
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Gaia DR2 | Stilism | sdss-wdms.org (29/04/2016) | Tremblay et al. 2011 | Vincent et al. 2024 | Simbad | Eisenstein et al. 2006 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 10 51 33.37 (0.05) | 10 51 33.35 | 10 51 33.37 (0.06) | 10 51 33.35 | 10 51 33.37 | 10 51 33.35 (0.05) | 10 51 33.35 | 10 51 32.47 | 10 51 33.36 | |||||
Declination | 66 34 00.69 (0.05) | 66 34 01.00 | 66 34 00.70 (0.06) | 66 34 00.98 | 66 34 00.69 | 66 34 01.01 (0.05) | 66 34 01.08 | 66 33 58.68 | 66 34 01.07 | |||||
Spectral type | DA+M | DA | DA | DA+M | DA+M | DA+ME | DA+M | DA+MS | ||||||
Effective temperature | [K] | 19416.0 (242) | 20810.0 (320) | 18954.0 (128) | 18646.0 (166) | |||||||||
log(g) | [cgs] | 7.64 (0.05) | 7.79 (0.05) | 7.40 (0.03) | 7.33 (0.03) | |||||||||
Mass | [M☉] | 0.44 (0.02) | 0.51 (0.02) | |||||||||||
log(Luminosity) | [L☉] | |||||||||||||
Cooling age | [Gyr] | 0.0380 | ||||||||||||
log(H/He) | ||||||||||||||
log(C/He) | ||||||||||||||
log(Ca/He) | ||||||||||||||
log(Ca/H) | ||||||||||||||
log(C/H) | ||||||||||||||
log(N/H) | ||||||||||||||
log(O/H) | ||||||||||||||
log(Na/H) | ||||||||||||||
log(Mg/H) | ||||||||||||||
log(Al/H) | ||||||||||||||
log(Si/H) | ||||||||||||||
log(P/H) | ||||||||||||||
log(S/H) | ||||||||||||||
log(Sc/H) | ||||||||||||||
log(Ti/H) | ||||||||||||||
log(Cr/H) | ||||||||||||||
log(Mn/H) | ||||||||||||||
log(Fe/H) | ||||||||||||||
log(Ni/H) | ||||||||||||||
Parallax | [mas] | 4.61 (0.06) | 4.52 (0.07) | 4.61 | 4.61 (0.06) | |||||||||
Distance | [pc] | 216.84 (3) | 221.17 (4) | 928.00 (137) | 216.84 | 216.84 (3) | ||||||||
Composition | H | |||||||||||||
Proper motion (right ascension) | [mas/yr] | 5.642285082 (0.06) | 5.664751987 (0.1) | 5.642 (0.06) | 3.9 | |||||||||
Proper motion (declination) | [mas/yr] | -20.3242466 (0.06) | -20.5977629 (0.1) | -20.324 (0.06) | -18.6 | |||||||||
Variability | ||||||||||||||
Magnetic | ||||||||||||||
Bd | [MG] | |||||||||||||
Infrared excess (disk) | ||||||||||||||
Binarity | WDMS | WDMS | yes | WDMS | WDMS | |||||||||
B magnitude | ||||||||||||||
V magnitude | ||||||||||||||
R magnitude | ||||||||||||||
I magnitude | ||||||||||||||
J magnitude | 15.49 (0.05) | |||||||||||||
H magnitude | 14.96 (0.07) | |||||||||||||
K magnitude | 14.53 (0.08) | |||||||||||||
u magnitude | 17.23 (0.008) | 17.27 | 17.23 (0.008) | 17.27 (0.02) | 17.26 | 17.24 (0.02) | ||||||||
g magnitude | 17.17 (0.004) | 17.10 | 17.16 (0.004) | 17.10 (0.03) | 17.16 | 17.09 (0.03) | ||||||||
r magnitude | 17.40 (0.005) | 17.42 | 17.39 (0.005) | 17.42 (0.02) | 17.41 | 17.41 (0.02) | ||||||||
i magnitude | 17.19 (0.006) | 17.19 | 17.19 (0.006) | 17.19 (0.01) | 17.19 | 17.19 (0.01) | ||||||||
z magnitude | 16.74 (0.01) | 16.72 | 16.75 (0.01) | 16.72 (0.02) | 16.71 | 16.73 (0.02) | ||||||||
G magnitude | 17.11 (0.006) | 17.13 | 17.11 | 17.11 (0.003) | ||||||||||
BP magnitude | 17.24 (0.006) | 17.23 | ||||||||||||
RP magnitude | 16.73 (0.005) | 16.74 | ||||||||||||
Pan g magnitude | 17.20 (0.005) | |||||||||||||
Pan r magnitude | 17.39 (0.005) | |||||||||||||
Pan i magnitude | 17.18 (0.003) | |||||||||||||
Pan z magnitude | 16.84 (0.005) | |||||||||||||
Pan y magnitude | 16.57 (0.005) | |||||||||||||
E(B-V) | 0.015 |
* Constant surface field
Spectra without link are available upon request
The Montreal White Dwarf Database is produced and maintained by Prof. Patrick Dufour (Université de Montréal) and Dr. Simon Blouin (University of Victoria). Please send database updates, corrections, suggestions or bug reports to patrick.dufour@umontreal.ca.