All names: WDJ101501.75+080611.24, Gaia DR2 3875652014008894720, Gaia DR2 3875651975353757440, WD 1012+083B, NLTT 23795, USNO-B1.0 0981-00220090, WD 1012+083.2, LP 549-32, ** LDS 3970B, WDS J10151+0806B, 10150+0806S, PSO J101501.527+080613.135, 2MASS J10150173+0806114, LSPM J1015+0806S, PSO J101501.500+080613.272
Parameter | Unit | Blouin et al. 2019 | MWDD H | MWDD HE | Pan-STARRS DR1 | Gaia DR2 | Limoges et al. 2015 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 10 15 01.44 (0.2) | 10 15 01.73 | 10 15 01.44 | 10 15 08.06 | ||||||
Declination | 08 06 13.70 (0.2) | 08 06 11.48 | 08 06 13.70 | 08 06 03.60 | ||||||
Spectral type | DC | DC | DC | DC | DC | DZ7 | ||||
Effective temperature | [K] | 4545.0 (20) | 4630.0 | 4317.0 | 4630.0 (102) | |||||
log(g) | [cgs] | 7.84 (0.03) | 7.90 | 7.66 | 7.95 (0.2) | |||||
Mass | [M☉] | 0.485 (0.01) | 0.518 | 0.38299999999999995 | 0.55 (0.1) | |||||
log(Luminosity) | [L☉] | -4.16 | ||||||||
Cooling age | [Gyr] | 5.7240 (0.3) | 6.1170 | 4.3460 | ||||||
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] | 33.55 (0.3) | 33.55 (0.3) | 34.50 (4) | 33.55 (0.3) | |||||
Distance | [pc] | 29.81 (0.3) | 29.81 (0.3) | 29.00 (3) | 29.81 (0.3) | |||||
Composition | H | |||||||||
Proper motion (right ascension) | [mas/yr] | -293.6703903 (0.3) | -288.0 | -293.6703903 | ||||||
Proper motion (declination) | [mas/yr] | 158.4346705 (0.4) | 169.0 | 158.4346705 | ||||||
Variability | ||||||||||
Magnetic | ||||||||||
Bd | [MG] | |||||||||
Infrared excess (disk) | ||||||||||
Binarity | yes | |||||||||
B magnitude | 17.90 | |||||||||
V magnitude | 17.77 | |||||||||
R magnitude | 17.00 | |||||||||
I magnitude | 17.20 | |||||||||
J magnitude | 16.06 (0.1) | 16.06 | ||||||||
H magnitude | 15.98 (0.2) | 15.98 | ||||||||
K magnitude | 15.22 (0.2) | 15.22 | ||||||||
u magnitude | 20.32 (0.05) | |||||||||
g magnitude | 18.33 (0.007) | |||||||||
r magnitude | 17.43 (0.005) | |||||||||
i magnitude | 17.09 (0.006) | |||||||||
z magnitude | 16.93 (0.01) | |||||||||
G magnitude | 17.51 | 17.51 | ||||||||
BP magnitude | 18.09 | 18.09 | ||||||||
RP magnitude | 16.79 | 16.79 | ||||||||
Pan g magnitude | 18.21 (0.001) | 18.20 (0.006) | ||||||||
Pan r magnitude | 17.43 (0.005) | 17.42 (0.005) | ||||||||
Pan i magnitude | 17.12 (0.003) | 17.14 (0.001) | ||||||||
Pan z magnitude | 17.01 (0.01) | 17.00 (0.005) | ||||||||
Pan y magnitude | 16.95 (0.02) | 16.96 (0.006) |
* Constant surface field
Spectra without link are available upon request
The Montreal White Dwarf Database is produced and maintained by Prof. Patrick Dufour at Université de Montréal. Please send database updates, corrections, suggestions or bug reports to dufourpa@astro.umontreal.ca.