All names: SDSS J080643.94+405838.1, J0806+4058, SDSS J080643.94+405837.7, WDJ080643.95+405838.24, SDSS J080643.94+405837.73, Gaia EDR3 921642532239821440, Gaia DR3 921642532239821440, Gaia DR2 921642532239821440
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR10 | Kilic et al. 2025 | Caron et al. 2023 | Gaia DR2 | Hollands et al. 2017 | Stilism | Kepler et al. 2015 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 08 06 43.94 (0.2) | 08 06 43.94 | 08 06 43.94 (0.2) | 08 06 43.94 | 08 06 43.95 (0.2) | 08 06 43.94 | ||||||||
Declination | 40 58 36.99 (0.1) | 40 58 37.74 | 40 58 37.03 (0.2) | 40 58 36.99 | 40 58 38.24 (0.1) | 40 58 37.03 | ||||||||
Spectral type | DZH | DZH | DZ | DZ | DZ | DZ | DZ | |||||||
Effective temperature | [K] | 6091.0 (38) | 6090.0 (42) | 6808.0 (80) | 6547.0 (19) | 6181.0 (214) | ||||||||
log(g) | [cgs] | 8.12 (0.02) | 8.17 (0.03) | 8.00 (0) | 8.14 (0.06) | |||||||||
Mass | [M☉] | 0.649 (0.02) | 0.679 (0.03) | 0.66 (0.06) | ||||||||||
log(Luminosity) | [L☉] | |||||||||||||
Cooling age | [Gyr] | 3.6100 | 2.1000 | |||||||||||
log(H/He) | -3.0 | -3.0 | ||||||||||||
log(C/He) | ||||||||||||||
log(Ca/He) | -9.16 | -9.1 | -8.49 | -8.802999999999999 (0.02) | ||||||||||
log(Ca/H) | ||||||||||||||
log(N/He) | ||||||||||||||
log(O/He) | ||||||||||||||
log(Na/He) | -8.33 | |||||||||||||
log(Mg/He) | -7.38 | |||||||||||||
log(Al/He) | ||||||||||||||
log(Si/He) | ||||||||||||||
log(P/He) | ||||||||||||||
log(S/He) | ||||||||||||||
log(Cl/He) | ||||||||||||||
log(Sc/He) | ||||||||||||||
log(Ti/He) | ||||||||||||||
log(V/He) | ||||||||||||||
log(Cr/He) | -9.11 | |||||||||||||
log(Mn/He) | ||||||||||||||
log(Fe/He) | -7.49 | |||||||||||||
log(Co/He) | ||||||||||||||
log(Ni/He) | -9.0 | |||||||||||||
log(Cu/He) | ||||||||||||||
log(Zn/He) | ||||||||||||||
log(Ga/He) | ||||||||||||||
log(Ge/He) | ||||||||||||||
log(Sr/He) | ||||||||||||||
Parallax | [mas] | 10.81 (0.2) | 11.10 (0.3) | 11.10 (0.3) | 10.81 | 10.81 (0.2) | 11.10 (0.3) | |||||||
Distance | [pc] | 92.54 (2) | 90.09 (3) | 90.11 (3) | 114.00 (16) | 92.54 | 92.54 (2) | 90.11 (3) | ||||||
Composition | He | He | He | |||||||||||
Proper motion (right ascension) | [mas/yr] | -6.772732318 (0.2) | -5.91411417 (0.5) | -6.773 (0.2) | -5.91411417 | |||||||||
Proper motion (declination) | [mas/yr] | -77.95290824 (0.2) | -77.97381556 (0.3) | -77.953 (0.2) | -77.97381556 | |||||||||
Variability | ||||||||||||||
Magnetic | yes | |||||||||||||
Bd | [MG] | 0.8 (0.03) | ||||||||||||
Infrared excess (disk) | ||||||||||||||
Binarity | ||||||||||||||
B magnitude | ||||||||||||||
V magnitude | ||||||||||||||
R magnitude | ||||||||||||||
I magnitude | ||||||||||||||
J magnitude | 18.33 (0.07) | |||||||||||||
H magnitude | ||||||||||||||
K magnitude | ||||||||||||||
u magnitude | 20.55 (0.06) | 20.63 (0.07) | 20.56 (0.06) | 20.55 (0.06) | 20.55 (0.06) | 20.56 (0.05) | ||||||||
g magnitude | 19.08 (0.01) | 19.08 (0.02) | 19.08 (0.01) | 19.07 (0.01) | 19.11 (0.009) | |||||||||
r magnitude | 18.76 (0.01) | 18.77 (0.01) | 18.76 (0.01) | 18.75 (0.01) | 18.77 (0.01) | |||||||||
i magnitude | 18.76 (0.01) | 18.77 (0.02) | 18.76 (0.01) | 18.76 (0.01) | 18.79 (0.01) | |||||||||
z magnitude | 18.84 (0.04) | 18.86 (0.04) | 18.84 (0.04) | 18.84 (0.04) | 18.85 (0.04) | |||||||||
G magnitude | 18.84 (0.04) | 18.85 | 18.84 | 18.84 (0.004) | 18.85 | |||||||||
BP magnitude | 19.10 (0.04) | 19.18 | 19.18 | |||||||||||
RP magnitude | 18.47 (0.04) | 18.48 | 18.48 | |||||||||||
Pan g magnitude | 19.03 (0.007) | 19.03 (0.007) | ||||||||||||
Pan r magnitude | 18.78 (0.008) | 18.78 (0.007) | ||||||||||||
Pan i magnitude | 18.79 (0.007) | 18.79 (0.007) | ||||||||||||
Pan z magnitude | 18.89 (0.02) | 18.89 (0.02) | ||||||||||||
Pan y magnitude | 18.87 (0.06) | 18.87 (0.06) | ||||||||||||
E(B-V) | 0.003 |
* 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.