All names: Gaia DR3 2747843836017055488, LP 525-17, WDJ002655.04+063538.87, Gaia EDR3 2747843836017055488, NLTT 1417, SDSS J002655.08+063538.1, PB 5951, SDSS J002655.08+063538.0, TIC 466440075, Gaia DR2 2747843836017055488, WDJ002655.04+063538.86, USNO-B1.0 0965-00004296, LSPM J0026+0635, 2MASS J00265505+0635395
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 00 26 55.14 (0.07) | 00 26 55.14 | 00 26 55.14 | 00 26 55.04 (0.07) | 00 26 55.14 | ||||||
Declination | 06 35 36.67 (0.05) | 06 35 36.73 | 06 35 36.67 | 06 35 38.87 (0.05) | 06 35 36.73 | ||||||
Spectral type | DA | DA | DA | ||||||||
Effective temperature | [K] | 7272.0 (40) | 7334.0 | 7063.0 | 7625.0 (78) | ||||||
log(g) | [cgs] | 8.02 (0.01) | 8.04 | 7.92 | 8.12 (0.02) | ||||||
Mass | [M☉] | 0.605 (0.009) | 0.615 | 0.53 | 0.667 (0.02) | ||||||
log(Luminosity) | [L☉] | ||||||||||
Cooling age | [Gyr] | 1.4150 | 1.3760 | ||||||||
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] | 17.17 (0.08) | 17.14 (0.1) | 17.17 | 17.17 (0.08) | 17.14 (0.1) | |||||
Distance | [pc] | 58.25 (0.3) | 58.35 (0.4) | 58.25 | 58.25 (0.3) | 58.35 (0.4) | |||||
Composition | H | ||||||||||
Proper motion (right ascension) | [mas/yr] | 90.72662088 (0.1) | 90.88408284 (0.2) | 90.727 (0.1) | 90.88408284 | ||||||
Proper motion (declination) | [mas/yr] | -137.7384522 (0.08) | -137.6163595 (0.1) | -137.738 (0.08) | -137.6163595 | ||||||
Variability | |||||||||||
Magnetic | |||||||||||
Bd | [MG] | ||||||||||
Infrared excess (disk) | |||||||||||
Binarity | |||||||||||
B magnitude | 17.50 | ||||||||||
V magnitude | |||||||||||
R magnitude | 17.00 | ||||||||||
I magnitude | |||||||||||
J magnitude | 16.59 (0.02) | ||||||||||
H magnitude | 15.93 (0.2) | ||||||||||
K magnitude | 16.41 (0.04) | ||||||||||
u magnitude | 17.80 (0.01) | 17.80 (0.01) | |||||||||
g magnitude | 17.32 (0.005) | 17.32 (0.005) | |||||||||
r magnitude | 17.16 (0.005) | 17.16 (0.005) | |||||||||
i magnitude | 17.13 (0.006) | 17.13 (0.006) | |||||||||
z magnitude | 17.17 (0.01) | 17.17 (0.01) | |||||||||
G magnitude | 17.13 (0.006) | 17.15 | 17.13 | 17.13 (0.003) | 17.15 | ||||||
BP magnitude | 17.29 (0.006) | 17.30 | 17.30 | ||||||||
RP magnitude | 16.83 (0.007) | 16.84 | 16.84 | ||||||||
Pan g magnitude | 17.29 (0.005) | ||||||||||
Pan r magnitude | 17.18 (0.009) | ||||||||||
Pan i magnitude | 17.16 (0.004) | ||||||||||
Pan z magnitude | 17.22 (0.004) | ||||||||||
Pan y magnitude | 17.27 (0.01) | ||||||||||
E(B-V) | 0.002 |
* 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.