All names: PSO J317.7087-21.4913, TIC 99495168, NLTT 50698, EGGR 581, LP 873-8, WD 2107-216, Gaia EDR3 6831993452567326592, WDJ211050.04-212922.52, 2MASS J21105002-2129216, Gaia DR3 6831993452567326592, J2110-2129, Gaia DR2 6831993452567326592, LHS 3636, UCAC4 343-203352
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | O'Brien et al. 2024 | Caron et al. 2023 | Blouin et al. 2019 | MWDD H | Gaia DR2 | Stilism | Bergeron et al. 2001 | Bergeron et al. 1997 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 21 10 50.13 (0.07) | 21 10 50.12 (0.09) | 21 10 50.13 | 21 10 50.04 (0.07) | 21 10 50.12 | 21 10 49.68 | |||||||||
Declination | -21 29 31.45 (0.05) | -21 29 31.17 (0.08) | -21 29 31.45 | -21 29 22.52 (0.05) | -21 29 31.17 | -21 28 54.84 | |||||||||
Spectral type | DA | DA | DA | DA | DA | DA | DA9 | DA9 | |||||||
Effective temperature | [K] | 5984.0 (59) | 6073.0 (12) | 5935.0 (35) | 5857.0 | 5830.0 (140) | 5840.0 (140) | 5855.0 (28) | |||||||
log(g) | [cgs] | 8.07 (0.03) | 8.12 (0.005) | 8.06 (0.02) | 8.03 | 8.40 (0.05) | 8.22 (0.05) | 8.02 (0.01) | |||||||
Mass | [M☉] | 0.631 (0.02) | 0.66 (0.005) | 0.622 (0.01) | 0.605 | 0.85 (0.03) | 0.73 (0.03) | 0.598 (0.009) | |||||||
log(Luminosity) | [L☉] | -4.02 (0.03) | -3.90 (0.03) | ||||||||||||
Cooling age | [Gyr] | 2.9000 | 2.6320 (0.1) | 2.5600 | 5.2400 (0.2) | 4.5200 (0.4) | |||||||||
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] | 31.39 (0.08) | 31.39 (0.08) | 31.44 (0.1) | 31.44 (0.1) | 31.44 (0.1) | 42.20 (2) | 37.00 (1) | 31.39 | 31.39 (0.08) | 31.44 (0.1) | 37.00 (1) | |||
Distance | [pc] | 31.86 (0.08) | 31.86 (0.08) | 31.81 (0.1) | 31.81 (0.1) | 31.81 (0.1) | 23.70 (0.8) | 27.03 (0.9) | 31.86 | 31.86 (0.08) | 31.81 (0.1) | 27.03 (0.7) | |||
Composition | H | H | H | H | H | ||||||||||
Proper motion (right ascension) | [mas/yr] | 76.97131487 (0.07) | 77.04212261 (0.2) | 76.971 (0.07) | 77.04212261 | ||||||||||
Proper motion (declination) | [mas/yr] | -558.1105599 (0.06) | -558.0357822 (0.1) | -558.111 (0.06) | -558.0357822 | ||||||||||
Variability | |||||||||||||||
Magnetic | |||||||||||||||
Bd | [MG] | ||||||||||||||
Infrared excess (disk) | |||||||||||||||
Binarity | |||||||||||||||
B magnitude | 17.39 | 17.39 | 17.44 (0.1) | ||||||||||||
V magnitude | 16.80 | 16.80 | 16.77 (0.01) | ||||||||||||
R magnitude | 16.45 | 16.45 | 16.36 (0.4) | ||||||||||||
I magnitude | 16.03 | 16.03 | |||||||||||||
J magnitude | 15.71 (0.006) | 15.69 (0.06) | 15.63 | 15.63 | 15.69 (0.06) | ||||||||||
H magnitude | 15.48 (0.1) | 15.48 (0.1) | 15.45 | 15.45 | 15.48 (0.1) | ||||||||||
K magnitude | 15.45 (0.02) | 15.70 (0.2) | 15.40 | 15.40 | 15.70 (0.2) | ||||||||||
u magnitude | |||||||||||||||
g magnitude | 16.98 (0.003) | ||||||||||||||
r magnitude | 16.65 (0.004) | ||||||||||||||
i magnitude | 16.52 (0.003) | ||||||||||||||
z magnitude | 16.50 (0.003) | ||||||||||||||
G magnitude | 16.64 (0.006) | 16.65 | 16.64 | 16.64 (0.003) | 16.65 | ||||||||||
BP magnitude | 16.97 (0.006) | 16.95 | 16.95 | ||||||||||||
RP magnitude | 16.21 (0.006) | 16.18 | 16.18 | ||||||||||||
Pan g magnitude | 16.98 (0.002) | 16.98 (0.002) | 16.98 (0.003) | ||||||||||||
Pan r magnitude | 16.65 (0.004) | 16.65 (0.004) | 16.65 (0.004) | ||||||||||||
Pan i magnitude | 16.52 (0.003) | 16.52 (0.003) | 16.52 (0.003) | ||||||||||||
Pan z magnitude | 16.50 (0.003) | 16.50 (0.003) | 16.50 (0.003) | ||||||||||||
Pan y magnitude | 16.50 (0.004) | 16.50 (0.004) | 16.50 (0.003) | ||||||||||||
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.