All names: Gaia DR3 721244821406496640, NLTT 24770, SDSS J103532.53+212603.6, PM J10355+2126, WDJ103532.60+212604.53, Gaia EDR3 721244821406496640, LSPM J1035+2126, PSO J158.8852+21.4340, 10355+2126, USNO-B1.0 1114-00191993, Gaia DR2 721244821406496640, TIC 171647302, WD 1032+216, GALEX J103532.5+212603, J1035+2126, LP 372-41, SDSS J103532.53+212603.5, 2MASS J10353263+2126048
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Kilic et al. 2025 | Hardy et al. 2023a | Caron et al. 2023 | Kilic et al. 2020 | Blouin et al. 2019 | MWDD H | Gaia DR2 | Stilism | Ferrario et al. 2015 | Limoges et al. 2015 | Kulebi et al. 2009 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 10 35 32.40 (0.07) | 10 35 32.53 | 10 35 32.40 (0.1) | 10 35 32.53 | 10 35 32.40 | 10 35 32.60 (0.07) | 10 35 32.40 | 10 35 32.40 | 10 35 32.53 | ||||||||||||
Declination | 21 26 01.54 (0.05) | 21 26 03.56 | 21 26 01.64 (0.08) | 21 26 03.52 | 21 26 01.54 | 21 26 04.53 (0.05) | 21 26 01.64 | 21 25 57.36 | 21 26 03.56 | ||||||||||||
Spectral type | DAH | DAH | DAH | DAH | DAH | DA | DA | DAH | DAH | DA | DAH | DAH | DAH7.2 | DAH | DA | ||||||
Effective temperature | [K] | 6949.0 (46) | 6881.6 (53) | 6797.0 (35) | 6949.0 (46) | 6965.0 (75) | 6993.0 | 7500.0 (500) | 7110.0 (144) | 7020.0 (64) | 6763.0 (31) | ||||||||||
log(g) | [cgs] | 8.08 (0.01) | 8.09 (0.02) | 8.02 (0.01) | 8.09 (0.01) | 8.10 (0.03) | 8.10 | 8.00 (0) | 8.00 (0) | 8.11 (0.02) | 9.99 (0.02) | ||||||||||
Mass | [M☉] | 0.64 (0.01) | 0.6435023023272883 (0.03) | 0.605 (0.01) | 0.645 (0.01) | 0.651 (0.02) | 0.653 | 0.59 (0.1) | 0.66 (0.01) | ||||||||||||
log(Luminosity) | [L☉] | -3.43 | |||||||||||||||||||
Cooling age | [Gyr] | 1.7500 | 1.7770 (0.1) | 1.7600 | |||||||||||||||||
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] | 18.77 (0.08) | 18.87 (0.1) | 18.87 (0.1) | 18.87 (0.1) | 18.77 | 18.77 (0.08) | 18.87 (0.1) | |||||||||||||
Distance | [pc] | 53.27 (0.2) | 52.99 (0.3) | 52.99 (0.3) | 52.99 (0.3) | 54.20 (7) | 53.27 | 53.27 (0.2) | 52.99 (0.3) | ||||||||||||
Composition | H | H | H | H | H | H | |||||||||||||||
Proper motion (right ascension) | [mas/yr] | -171.6285512 (0.08) | -171.6741939 (0.2) | -77.0 | -171.629 (0.08) | -171.674 | |||||||||||||||
Proper motion (declination) | [mas/yr] | -186.5381919 (0.07) | -186.6898726 (0.2) | -145.0 | -186.538 (0.07) | -186.69 | |||||||||||||||
Variability | |||||||||||||||||||||
Magnetic | yes | yes | yes | yes | |||||||||||||||||
Bd | [MG] | 2.628171614223491 | 2.96 (0.3) | 2.96 (0.3) | |||||||||||||||||
Infrared excess (disk) | |||||||||||||||||||||
Binarity | |||||||||||||||||||||
B magnitude | 17.70 | ||||||||||||||||||||
V magnitude | |||||||||||||||||||||
R magnitude | 16.20 | ||||||||||||||||||||
I magnitude | |||||||||||||||||||||
J magnitude | 16.63 (0.02) | 16.50 (0.1) | 16.50 | 16.50 (0.1) | |||||||||||||||||
H magnitude | 16.83 (0.3) | 16.83 (0.3) | 16.83 | 16.83 (0.3) | |||||||||||||||||
K magnitude | 15.60 (0.03) | 15.60 | |||||||||||||||||||
u magnitude | 17.96 (0.01) | 17.96 (0.01) | 17.96 (0.01) | 17.96 (0.01) | 17.98 | 18.00 (0.02) | |||||||||||||||
g magnitude | 17.39 (0.005) | 17.38 (0.003) | 17.39 (0.005) | 17.40 | 17.40 (0.02) | ||||||||||||||||
r magnitude | 17.21 (0.005) | 17.22 (0.004) | 17.21 (0.005) | 17.23 | 17.20 (0.01) | ||||||||||||||||
i magnitude | 17.19 (0.006) | 17.18 (0.009) | 17.19 (0.006) | 17.19 | 17.17 (0.02) | ||||||||||||||||
z magnitude | 17.21 (0.01) | 17.21 (0.01) | 17.21 (0.01) | 17.21 | 17.20 (0.03) | ||||||||||||||||
G magnitude | 17.19 (0.008) | 17.21 | 17.19 | 17.19 (0.003) | 17.21 | ||||||||||||||||
BP magnitude | 17.38 (0.008) | 17.36 | 17.36 | ||||||||||||||||||
RP magnitude | 16.87 (0.01) | 16.87 | 16.87 | ||||||||||||||||||
Pan g magnitude | 17.38 (0.003) | 17.38 (0.003) | 17.38 (0.003) | ||||||||||||||||||
Pan r magnitude | 17.22 (0.005) | 17.22 (0.005) | 17.22 (0.005) | ||||||||||||||||||
Pan i magnitude | 17.18 (0.01) | 17.18 (0.009) | 17.18 (0.009) | ||||||||||||||||||
Pan z magnitude | 17.24 (0.03) | 17.24 (0.02) | 17.24 (0.02) | ||||||||||||||||||
Pan y magnitude | 17.26 (0.02) | 17.26 (0.02) | 17.26 (0.02) | ||||||||||||||||||
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.