All names: TIC 266474478, LSPM J0905+7314, Gaia DR2 1123700235048742016, PM J09055+7314, WD 0900+734, PSO J136.3823+73.2466, Gaia EDR3 1123700235048742016, G 252-27, 2MASS J09053288+7314546, WDJ090532.93+731454.95, GJ 3529, EGGR 349, Gaia DR3 1123700235048742016, LHS 2101, WD 0900+73, NLTT 20850, LP 36-115, USNO-B1.0 1632-00076053, 09055+7314, J0905+7314
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | O'Brien et al. 2024 | Caron et al. 2023 | McCleery et al. 2020 | Blouin et al. 2019 | Gaia DR2 | Stilism | Limoges et al. 2015 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 09 05 31.68 (0.03) | 09 05 31.72 (0.05) | 09 05 31.72 (0.05) | 09 05 31.68 | 09 05 32.93 (0.03) | 09 05 31.72 | 09 05 34.61 | |||||||
Declination | 73 14 47.38 (0.05) | 73 14 47.62 (0.06) | 73 14 47.62 (0.06) | 73 14 47.38 | 73 14 54.95 (0.05) | 73 14 47.62 | 73 15 02.16 | |||||||
Spectral type | DC | DC | DC | DC | DC | DA: | DC9 | DC9 | ||||||
Effective temperature | [K] | 5065.0 (26) | 5199.0 (11) | 5106.4 (22) | 5170.0 (25) | 5120.0 (609) | 5171.0 (21) | |||||||
log(g) | [cgs] | 7.93 (0.02) | 8.03 (0.005) | 7.96 (0.02) | 8.01 (0.02) | 8.00 (0) | 8.00 (0.01) | |||||||
Mass | [M☉] | 0.527 (0.01) | 0.598 (0.005) | 0.588 (0.01) | 0.58 (0.1) | 0.58 (0.008) | ||||||||
log(Luminosity) | [L☉] | -4.01 | ||||||||||||
Cooling age | [Gyr] | 4.9800 | 4.9810 (0.3) | |||||||||||
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] | 38.96 (0.06) | 38.96 (0.06) | 38.89 (0.07) | 38.89 (0.07) | 38.89 (0.07) | 38.89 (0.07) | 38.96 | 38.96 (0.06) | 38.89 (0.07) | ||||
Distance | [pc] | 25.67 (0.04) | 25.67 (0.04) | 25.71 (0.05) | 25.72 (0.05) | 25.72 (0.05) | 25.72 (0.05) | 25.90 (6) | 25.67 | 25.67 (0.04) | 25.72 (0.05) | |||
Composition | H | He | H | H | ||||||||||
Proper motion (right ascension) | [mas/yr] | -337.9130689 (0.05) | -337.9195821 (0.09) | -337.913 (0.05) | -337.9195821 | |||||||||
Proper motion (declination) | [mas/yr] | -472.6964594 (0.06) | -472.8704685 (0.1) | -472.696 (0.06) | -472.8704685 | |||||||||
Variability | ||||||||||||||
Magnetic | ||||||||||||||
Bd | [MG] | |||||||||||||
Infrared excess (disk) | ||||||||||||||
Binarity | ||||||||||||||
B magnitude | 17.20 | |||||||||||||
V magnitude | ||||||||||||||
R magnitude | 16.50 | |||||||||||||
I magnitude | ||||||||||||||
J magnitude | 15.56 (0.06) | 15.56 (0.06) | 15.56 (0.06) | |||||||||||
H magnitude | 15.27 (0.1) | 15.27 (0.1) | 15.27 (0.1) | |||||||||||
K magnitude | 15.13 (0.1) | 15.13 (0.1) | 15.13 (0.1) | |||||||||||
u magnitude | ||||||||||||||
g magnitude | 17.28 (0.003) | |||||||||||||
r magnitude | 16.73 (0.002) | |||||||||||||
i magnitude | 16.51 (0.003) | |||||||||||||
z magnitude | 16.43 (0.004) | |||||||||||||
G magnitude | 16.75 (0.004) | 16.77 | 16.77 | 16.75 | 16.75 (0.003) | 16.77 | ||||||||
BP magnitude | 17.19 (0.004) | 17.22 | 17.22 | |||||||||||
RP magnitude | 16.15 (0.003) | 16.17 | 16.17 | |||||||||||
Pan g magnitude | 17.28 (0.003) | 17.28 (0.003) | 17.28 (0.003) | |||||||||||
Pan r magnitude | 16.73 (0.003) | 16.73 (0.002) | 16.73 (0.002) | |||||||||||
Pan i magnitude | 16.51 (0.002) | 16.51 (0.003) | 16.51 (0.003) | |||||||||||
Pan z magnitude | 16.43 (0.005) | 16.43 (0.004) | 16.43 (0.004) | |||||||||||
Pan y magnitude | 16.40 (0.005) | 16.40 (0.005) | 16.40 (0.005) | |||||||||||
E(B-V) | 0.001 |
* 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.