All names: WDJ023759.15+163812.95, 2MASS J02375916+1638138, PSO J039.4963+16.6359, Gaia EDR3 81606375784491520, NLTT 8525, Gaia DR2 81606375784491520, Gaia DR3 81606375784491520, USNO-B1.0 1066-00026276, J0237+1638, TIC 408852780, LP 410-67, PM J02379+1638, 02379+1638, LSPM J0237+1638
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | O'Brien et al. 2024 | Caron et al. 2023 | McCleery et al. 2020 | Blouin et al. 2019 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Limoges et al. 2015 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 02 37 59.11 (0.1) | 02 37 59.11 (0.1) | 02 37 59.11 (0.1) | 02 37 59.11 | 02 37 59.15 (0.1) | 02 37 59.11 | |||||||||
Declination | 16 38 07.97 (0.07) | 16 38 08.12 (0.08) | 16 38 08.12 (0.08) | 16 38 07.97 | 16 38 12.95 (0.07) | 16 38 08.12 | |||||||||
Spectral type | DC | DC | DC | DC | DC | DC | DC | DA: | DC | ||||||
Effective temperature | [K] | 5441.0 (70) | 5312.0 (25) | 5427.0 (40) | 5250.0 (55) | 5554.0 | 5272.0 | 5150.0 (607) | 5650.0 (44) | ||||||
log(g) | [cgs] | 8.04 (0.05) | 7.96 (0.01) | 8.04 (0.03) | 7.93 (0.03) | 8.11 | 7.93 | 8.00 (0) | 8.17 (0.02) | ||||||
Mass | [M☉] | 0.595 (0.03) | 0.545 (0.01) | 0.53 (0.01) | 0.656 | 0.53 | 0.57 (0.1) | 0.692 (0.01) | |||||||
log(Luminosity) | [L☉] | -4.00 | |||||||||||||
Cooling age | [Gyr] | 4.5100 | 4.2840 (0.3) | 4.0150 | 4.1870 | ||||||||||
log(H/He) | |||||||||||||||
log(C/He) | |||||||||||||||
log(Ca/He) | |||||||||||||||
log(Ca/H) | |||||||||||||||
log(N/He) | |||||||||||||||
log(O/He) | |||||||||||||||
log(Na/He) | |||||||||||||||
log(Mg/He) | |||||||||||||||
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) | |||||||||||||||
log(Mn/He) | |||||||||||||||
log(Fe/He) | |||||||||||||||
log(Co/He) | |||||||||||||||
log(Ni/He) | |||||||||||||||
log(Cu/He) | |||||||||||||||
log(Zn/He) | |||||||||||||||
log(Ga/He) | |||||||||||||||
log(Ge/He) | |||||||||||||||
log(Sr/He) | |||||||||||||||
Parallax | [mas] | 31.34 (0.1) | 31.34 (0.1) | 31.24 (0.1) | 31.24 (0.1) | 31.25 (0.1) | 31.24 (0.1) | 31.34 | 31.34 (0.1) | 31.24 (0.1) | |||||
Distance | [pc] | 31.91 (0.1) | 31.91 (0.1) | 32.01 (0.1) | 32.01 (0.1) | 32.01 (0.1) | 32.01 (0.1) | 30.70 (5) | 31.91 | 31.91 (0.1) | 32.01 (0.1) | ||||
Composition | He | He | He | He | |||||||||||
Proper motion (right ascension) | [mas/yr] | -41.8048972 (0.1) | -41.59016625 (0.2) | -41.805 (0.1) | -41.59016625 | ||||||||||
Proper motion (declination) | [mas/yr] | -311.5274578 (0.08) | -311.4818881 (0.1) | -311.527 (0.08) | -311.4818881 | ||||||||||
Variability | |||||||||||||||
Magnetic | |||||||||||||||
Bd | [MG] | ||||||||||||||
Infrared excess (disk) | |||||||||||||||
Binarity | |||||||||||||||
B magnitude | 17.60 | ||||||||||||||
V magnitude | |||||||||||||||
R magnitude | 16.80 | ||||||||||||||
I magnitude | |||||||||||||||
J magnitude | 16.04 (0.01) | 15.97 (0.1) | 15.97 | 15.97 (0.1) | |||||||||||
H magnitude | 15.83 (0.2) | 15.83 (0.2) | 15.83 | 15.83 (0.2) | |||||||||||
K magnitude | 14.88 (0.03) | 14.88 | |||||||||||||
u magnitude | |||||||||||||||
g magnitude | 17.46 (0.006) | ||||||||||||||
r magnitude | 17.03 (0.005) | ||||||||||||||
i magnitude | 16.86 (0.005) | ||||||||||||||
z magnitude | 16.81 (0.005) | ||||||||||||||
G magnitude | 17.04 (0.01) | 17.06 | 17.06 | 17.04 | 17.04 (0.003) | 17.06 | |||||||||
BP magnitude | 17.41 (0.01) | 17.41 | 17.41 | ||||||||||||
RP magnitude | 16.52 (0.009) | 16.52 | 16.52 | ||||||||||||
Pan g magnitude | 17.46 (0.006) | 17.46 (0.006) | 17.46 (0.006) | ||||||||||||
Pan r magnitude | 17.03 (0.005) | 17.03 (0.005) | 17.03 (0.005) | ||||||||||||
Pan i magnitude | 16.86 (0.006) | 16.86 (0.005) | 16.86 (0.005) | ||||||||||||
Pan z magnitude | 16.81 (0.004) | 16.81 (0.005) | 16.80 (0.005) | ||||||||||||
Pan y magnitude | 16.79 (0.009) | 16.79 (0.01) | 16.79 (0.01) | ||||||||||||
E(B-V) | 0.000 |
* 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.