All names: LAMOST J134259.84+022209.6, SDSS J134259.83+022209.4, LBQS 1340+0237, PSO J134259.831+022209.482, Gaia DR2 3665169715669748096, SDSS J134259.84+022209.62
Parameter | Unit | MWDD H | Pan-STARRS DR1 | Gaia DR2 | Kepler et al. 2015 | SDSS DR10 | Simbad |
---|---|---|---|---|---|---|---|
Right ascension | 13 42 59.83 (0.1) | 13 42 59.84 | 13 42 59.84 | ||||
Declination | 02 22 09.39 (0.1) | 02 22 09.44 | 02 22 09.44 | ||||
Spectral type | DA | DA | DA | ||||
Effective temperature | [K] | 13856.0 | 22654.0 (139) | ||||
log(g) | [cgs] | 7.46 | 7.99 (0.02) | ||||
Mass | [M☉] | 0.358 | 0.623 (0.01) | ||||
log(Luminosity) | [L☉] | ||||||
Cooling age | [Gyr] | 0.1288 | |||||
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] | 4.03 (0.2) | |||||
Distance | [pc] | 247.99 (10) | |||||
Composition | H | ||||||
Proper motion (right ascension) | [mas/yr] | -12.5507605637 (0.3) | -11.0 | ||||
Proper motion (declination) | [mas/yr] | -11.0837443149 (0.2) | -6.0 | ||||
Variability | |||||||
Magnetic | |||||||
Bd | [MG] | ||||||
Infrared excess (disk) | |||||||
Binarity | |||||||
B magnitude | |||||||
V magnitude | |||||||
R magnitude | |||||||
I magnitude | |||||||
J magnitude | 17.96 | ||||||
H magnitude | 18.10 | ||||||
K magnitude | 18.10 | ||||||
u magnitude | 17.64 (0.02) | 17.66 (0.01) | 17.66 | ||||
g magnitude | 17.52 (0.01) | 17.50 (0.005) | 17.50 | ||||
r magnitude | 17.81 (0.02) | 17.79 (0.006) | 17.79 | ||||
i magnitude | 18.07 (0.02) | 18.05 (0.009) | 18.05 | ||||
z magnitude | 18.31 (0.03) | 18.30 (0.03) | 18.30 | ||||
G magnitude | 17.69 | ||||||
BP magnitude | 17.63 | ||||||
RP magnitude | 17.78 | ||||||
Pan g magnitude | 17.55 (0.005) | ||||||
Pan r magnitude | 17.81 (0.006) | ||||||
Pan i magnitude | 18.08 (0.004) | ||||||
Pan z magnitude | 18.31 (0.008) | ||||||
Pan y magnitude | 18.48 (0.03) |
* 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.