All names: CCDM J22196+2122B, PM J22194+2122, NLTT 53526, LP 460-3, WD 2217+211, LSPM J2219+2122W, BD+20 5125B, TIC 353035668, LP 460-003, J2219+2122, ** LDS 4956B, PSO J334.8703+21.3730, Gaia EDR3 1778836056545324160, USNO-B1.0 1113-00582739, WDJ221928.57+212220.58, Gaia DR3 1778836056545324160, 22194+2122, SDSS J221928.69+212221.5, WDS J22196+2122B, 2MASS J22192853+2122194, Gaia DR2 1778836056545324160
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | Caron et al. 2023 | Blouin et al. 2019 | MWDD H | MWDD HE | Gaia DR2 | Tremblay et al. 2017 | Stilism | Limoges et al. 2015 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 22 19 28.99 (0.1) | 22 19 28.98 (0.1) | 22 19 28.99 | 22 19 28.57 (0.1) | 22 19 28.98 | 22 19 27.62 | ||||||||||
Declination | 21 22 23.87 (0.1) | 21 22 23.76 (0.2) | 21 22 23.87 | 21 22 20.57 (0.1) | 21 22 23.76 | 21 22 05.16 | ||||||||||
Spectral type | DC | DC | DC | DC | DC | DC | DC | DC: | DC9 | DC9 | ||||||
Effective temperature | [K] | 4748.0 (23) | 4764.0 (19) | 4395.0 (90) | 5229.0 | 4927.0 | 4600.0 (355) | 4796.0 (51) | ||||||||
log(g) | [cgs] | 7.33 (0.07) | 7.16 (0.02) | 6.79 (0.1) | 7.78 | 7.56 | 8.00 (0) | 7.17 (0.04) | ||||||||
Mass | [M☉] | 0.319 (0.06) | 0.21 (0.007) | 0.08 (0.04) | 0.457 | 0.339 | 0.58 (0.1) | 0.212 (0.01) | ||||||||
log(Luminosity) | [L☉] | -4.19 | ||||||||||||||
Cooling age | [Gyr] | 1.8100 | 1.6100 (0.2) | 2.5410 | 2.5620 | |||||||||||
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] | 18.52 (0.1) | 18.61 (0.2) | 18.61 (0.2) | 18.61 (0.2) | 18.76 (0.4) | 18.52 | 18.52 (0.1) | 18.61 (0.2) | 20.10 (2) | ||||||
Distance | [pc] | 54.01 (0.4) | 53.73 (0.5) | 53.72 (0.5) | 53.72 (0.5) | 53.30 (1) | 32.00 (7) | 54.01 | 54.01 (0.4) | 53.72 (0.5) | 49.75 (5) | |||||
Composition | H | H | He | H | ||||||||||||
Proper motion (right ascension) | [mas/yr] | 368.3824724 (0.1) | 368.0949353 (0.2) | 368.382 (0.1) | 368.0949353 | |||||||||||
Proper motion (declination) | [mas/yr] | 205.8519058 (0.1) | 205.3760083 (0.3) | 205.852 (0.1) | 205.3760083 | |||||||||||
Variability | ||||||||||||||||
Magnetic | ||||||||||||||||
Bd | [MG] | |||||||||||||||
Infrared excess (disk) | ||||||||||||||||
Binarity | yes | |||||||||||||||
B magnitude | 19.10 | |||||||||||||||
V magnitude | 17.69 (0.05) | 18.30 | ||||||||||||||
R magnitude | 17.40 | |||||||||||||||
I magnitude | ||||||||||||||||
J magnitude | 16.41 (0.02) | 16.45 (0.1) | 16.45 (0.1) | |||||||||||||
H magnitude | ||||||||||||||||
K magnitude | 16.02 (0.3) | 16.02 (0.3) | 16.02 (0.3) | |||||||||||||
u magnitude | 20.27 (0.03) | 20.27 (0.04) | 20.27 (0.04) | |||||||||||||
g magnitude | 18.42 (0.009) | 18.54 (0.007) | ||||||||||||||
r magnitude | 17.71 (0.004) | 17.73 (0.006) | ||||||||||||||
i magnitude | 17.43 (0.005) | 17.41 (0.007) | ||||||||||||||
z magnitude | 17.32 (0.009) | 17.24 (0.01) | ||||||||||||||
G magnitude | 17.75 (0.02) | 17.77 | 17.67 (0.004) | 17.75 | 17.75 (0.003) | 17.77 | ||||||||||
BP magnitude | 18.35 (0.02) | 18.34 | 18.34 | |||||||||||||
RP magnitude | 17.10 (0.01) | 17.10 | 17.10 | |||||||||||||
Pan g magnitude | 18.42 (0.009) | 18.42 (0.009) | 18.42 (0.009) | |||||||||||||
Pan r magnitude | 17.71 (0.004) | 17.71 (0.004) | 17.71 (0.004) | |||||||||||||
Pan i magnitude | 17.43 (0.004) | 17.43 (0.004) | 17.43 (0.005) | |||||||||||||
Pan z magnitude | 17.32 (0.007) | 17.32 (0.007) | 17.32 (0.009) | |||||||||||||
Pan y magnitude | 17.28 (0.03) | 17.28 (0.03) | 17.28 (0.02) | |||||||||||||
E(B-V) | 0.004 |
* 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.