All names: 2QZ J113313.2-013825, SDSS J113313.26-013824.5, WISE J113313.24-013824.5, TIC 173164987, WISEA J113313.24-013824.6, 2MASS J11331324-0138249, EPIC 201354365, WD 1130-013, Gaia EDR3 3793645695165784448, USNO-B1.0 0883-00233920
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Simbad | White Dwarf Catalog (McCook & Sion 1999) |
---|---|---|---|---|---|
Right ascension | 11 33 13.25 (1) | 11 33 13.25 (260) | 11 33 12.53 | ||
Declination | -01 38 24.74 (1) | -01 38 24.91 (210) | -01 38 28.68 | ||
Spectral type | DA3.0+dM | DA3.0+dM | |||
Effective temperature | [K] | ||||
log(g) | [cgs] | ||||
Mass | [M☉] | ||||
log(Luminosity) | [L☉] | ||||
Cooling age | [Gyr] | ||||
log(H/He) | |||||
log(C/He) | |||||
log(Ca/He) | |||||
log(Ca/H) | |||||
Parallax | [mas] | ||||
Distance | [pc] | ||||
Composition | |||||
Proper motion (right ascension) | [mas/yr] | 1.0 (3) | |||
Proper motion (declination) | [mas/yr] | -8.0 (3) | |||
Variability | |||||
Magnetic | |||||
Bd | [MG] | ||||
Infrared excess (disk) | |||||
Binarity | yes | ||||
B magnitude | 18.70 | ||||
V magnitude | 19.20 | ||||
R magnitude | 18.90 | ||||
I magnitude | |||||
J magnitude | 16.23 (0.1) | ||||
H magnitude | 15.75 (0.1) | ||||
K magnitude | 15.48 (0.2) | ||||
u magnitude | 19.28 (0.03) | ||||
g magnitude | 19.13 (0.01) | ||||
r magnitude | 19.00 (0.01) | ||||
i magnitude | 18.23 (0.01) | ||||
z magnitude | 17.66 (0.02) | ||||
G magnitude | 19.19 (0.04) | ||||
BP magnitude | 19.12 (0.04) | ||||
RP magnitude | 17.80 (0.02) | ||||
Pan g magnitude | 19.17 (0.01) | ||||
Pan r magnitude | 19.05 (0.009) | ||||
Pan i magnitude | 18.26 (0.01) | ||||
Pan z magnitude | 17.79 (0.004) | ||||
Pan y magnitude | 17.53 (0.02) | ||||
E(B-V) |
* 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.