All names: LSPM J1857+5330, LP 141-14, WDJ185739.34+533033.30, 18576+5330, WD 1856+534, Gaia EDR3 2146576589564898688, 2MASS J18573936+5330332, ** LDS 4802C, Gaia DR2 2146576589564898688, PSO J284.4153+53.5090, TIC 267574918, WDS J18576+5331C, PM J18576+5330, USNO-B1.0 1435-00280850, NLTT 47263, J1857+5330, CNS5 4719, TOI-1690, Gaia DR3 2146576589564898688
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 | White Dwarf Catalog (McCook & Sion 1999) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 18 57 39.78 (0.06) | 18 57 39.76 (0.08) | 18 57 39.76 (0.08) | 18 57 39.78 | 18 57 39.34 (0.06) | 18 57 39.76 | 18 57 36.34 | |||||||||
Declination | 53 30 32.46 (0.05) | 53 30 32.49 (0.08) | 53 30 32.49 (0.08) | 53 30 32.46 | 53 30 33.30 (0.05) | 53 30 32.49 | 53 31 06.96 | |||||||||
Spectral type | DC | DC | DC | DC | DC | DC | DC | DC | DC | DC | ||||||
Effective temperature | [K] | 4738.0 (40) | 4833.0 (12) | 4707.4 (22) | 4430.0 (60) | 4784.0 | 4464.0 | 5570.0 (546) | 4814.0 (26) | |||||||
log(g) | [cgs] | 7.88 (0.03) | 7.97 (0.006) | 7.87 (0.02) | 7.69 (0.03) | 7.92 | 7.69 | 8.00 (0) | 7.94 (0.01) | |||||||
Mass | [M☉] | 0.507 (0.02) | 0.56 (0.005) | 0.396 (0.01) | 0.533 | 0.398 | 0.58 (0.1) | 0.54 (0.01) | ||||||||
log(Luminosity) | [L☉] | -3.86 | ||||||||||||||
Cooling age | [Gyr] | 6.3400 | 4.2550 (0.2) | 5.7860 | 4.1890 | |||||||||||
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] | 40.39 (0.05) | 40.39 (0.05) | 40.40 (0.07) | 40.40 (0.07) | 40.40 (0.07) | 40.40 (0.07) | 40.39 | 40.39 (0.05) | 40.40 (0.07) | ||||||
Distance | [pc] | 24.76 (0.03) | 24.76 (0.03) | 24.75 (0.04) | 24.75 (0.04) | 24.75 (0.04) | 24.75 (0.04) | 31.80 (6) | 24.76 | 24.76 (0.03) | 24.75 (0.04) | |||||
Composition | H | He | H | |||||||||||||
Proper motion (right ascension) | [mas/yr] | 240.7492369 (0.07) | 240.7585621 (0.1) | 240.749 (0.07) | 240.7585621 | |||||||||||
Proper motion (declination) | [mas/yr] | -52.47014066 (0.06) | -52.51395749 (0.1) | -52.47 (0.06) | -52.51395749 | |||||||||||
Variability | ||||||||||||||||
Magnetic | ||||||||||||||||
Bd | [MG] | |||||||||||||||
Infrared excess (disk) | ||||||||||||||||
Binarity | ||||||||||||||||
B magnitude | 17.60 | |||||||||||||||
V magnitude | ||||||||||||||||
R magnitude | 16.40 | |||||||||||||||
I magnitude | ||||||||||||||||
J magnitude | 15.57 (0.01) | 15.68 (0.06) | 15.68 (0.06) | |||||||||||||
H magnitude | 15.43 (0.09) | 15.43 (0.09) | 15.43 (0.09) | |||||||||||||
K magnitude | 15.55 (0.2) | 15.55 (0.2) | 15.55 (0.2) | |||||||||||||
u magnitude | ||||||||||||||||
g magnitude | 17.60 (0.005) | |||||||||||||||
r magnitude | 16.91 (0.003) | |||||||||||||||
i magnitude | 16.62 (0.004) | |||||||||||||||
z magnitude | 16.52 (0.003) | |||||||||||||||
G magnitude | 16.94 (0.008) | 16.96 | 16.96 | 16.94 | 16.94 (0.003) | 16.96 | ||||||||||
BP magnitude | 17.47 (0.008) | 17.50 | 17.50 | |||||||||||||
RP magnitude | 16.26 (0.004) | 16.28 | 16.28 | |||||||||||||
Pan g magnitude | 17.60 (0.005) | 17.60 (0.005) | 17.60 (0.005) | |||||||||||||
Pan r magnitude | 16.91 (0.003) | 16.91 (0.003) | 16.91 (0.003) | |||||||||||||
Pan i magnitude | 16.62 (0.003) | 16.62 (0.004) | 16.62 (0.004) | |||||||||||||
Pan z magnitude | 16.52 (0.003) | 16.52 (0.003) | 16.52 (0.003) | |||||||||||||
Pan y magnitude | 16.47 (0.008) | 16.47 (0.006) | 16.47 (0.006) | |||||||||||||
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.