All names: WD 1040+520, USNO-B1.0 1417-00230820, SBSS 1040+520, PSO J104350.869+514508.788, Gaia DR2 837038411017250944, SDSS J104350.84+514508.69
Parameter | Unit | MWDD H | Pan-STARRS DR1 | Gaia DR2 | Kepler et al. 2016 | SDSS DR12 | Simbad |
---|---|---|---|---|---|---|---|
Right ascension | 10 43 50.87 (0.06) | 10 43 50.85 | 10 43 50.85 | ||||
Declination | 51 45 08.71 (0.1) | 51 45 08.69 | 51 45 08.69 | ||||
Spectral type | DA | DA | DA | ||||
Effective temperature | [K] | 18773.0 | 19926.0 (103) | ||||
log(g) | [cgs] | 8.22 | 8.20 (0.02) | ||||
Mass | [M☉] | 0.7509999999999999 | 0.727 (0.01) | ||||
log(Luminosity) | [L☉] | ||||||
Cooling age | [Gyr] | 0.1408 | |||||
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] | 4.60 (0.2) | |||||
Distance | [pc] | 217.20 (8) | |||||
Composition | H | ||||||
Proper motion (right ascension) | [mas/yr] | 7.867676039 (0.2) | 3.0 | ||||
Proper motion (declination) | [mas/yr] | -0.4201820405 (0.3) | -1.0 | ||||
Variability | |||||||
Magnetic | |||||||
Bd | [MG] | ||||||
Infrared excess (disk) | |||||||
Binarity | |||||||
B magnitude | 19.00 | ||||||
V magnitude | |||||||
R magnitude | 17.30 | ||||||
I magnitude | |||||||
J magnitude | |||||||
H magnitude | |||||||
K magnitude | |||||||
u magnitude | 17.82 (0.03) | 17.79 (0.01) | 17.82 | ||||
g magnitude | 17.70 (0.02) | 17.69 (0.005) | 17.70 | ||||
r magnitude | 18.09 (0.02) | 18.09 (0.007) | 18.09 | ||||
i magnitude | 18.40 (0.02) | 18.39 (0.01) | 18.40 | ||||
z magnitude | 18.70 (0.04) | 18.71 (0.04) | 18.70 | ||||
G magnitude | 17.94 | ||||||
BP magnitude | 17.81 | ||||||
RP magnitude | 18.06 | ||||||
Pan g magnitude | 17.77 (0.009) | ||||||
Pan r magnitude | 18.09 (0.006) | ||||||
Pan i magnitude | 18.42 (0.006) | ||||||
Pan z magnitude | 18.68 (0.02) | ||||||
Pan y magnitude | 18.82 (0.02) |
* 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.