All names: Gaia DR2 2522906262603157760, SDSS J004955.17-071240.8, SDSS J004955.17-071240.9, Gaia EDR3 2522906262603157760, Gaia DR3 2522906262603157760, WDJ004954.98-071240.64
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Gaia DR2 | Stilism | Simbad | Gentile Fusillo et al. 2018 |
---|---|---|---|---|---|---|---|
Right ascension | 00 49 55.30 (0.5) | 00 49 55.29 | 00 49 54.98 (0.5) | 00 49 55.29 | |||
Declination | -07 12 41.10 (0.3) | -07 12 41.09 | -07 12 40.64 (0.3) | -07 12 41.09 | |||
Spectral type | CND | ||||||
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] | 12.92 (0.5) | 13.22 (0.7) | 12.92 (0.5) | 13.22 (0.7) | ||
Distance | [pc] | 77.41 (3) | 75.65 (4) | 77.41 (3) | 75.65 (4) | ||
Composition | |||||||
Proper motion (right ascension) | [mas/yr] | 292.7787283 (1) | 293.4691731 (1) | 292.779 (1) | 293.4691731 | ||
Proper motion (declination) | [mas/yr] | -28.96905049 (0.5) | -28.7308383 (0.7) | -28.969 (0.5) | -28.7308383 | ||
Variability | |||||||
Magnetic | |||||||
Bd | [MG] | ||||||
Infrared excess (disk) | |||||||
Binarity | |||||||
B magnitude | |||||||
V magnitude | |||||||
R magnitude | |||||||
I magnitude | |||||||
J magnitude | |||||||
H magnitude | |||||||
K magnitude | |||||||
u magnitude | 24.00 (1) | 24.00 (1) | |||||
g magnitude | 20.60 (0.03) | 20.60 (0.03) | |||||
r magnitude | 19.72 (0.02) | 19.72 (0.02) | |||||
i magnitude | 19.39 (0.02) | 19.39 (0.02) | |||||
z magnitude | 19.33 (0.07) | 19.33 (0.07) | |||||
G magnitude | 19.72 (0.08) | 19.76 | 19.72 (0.004) | 19.76 | |||
BP magnitude | 20.26 (0.08) | 20.34 | 20.34 | ||||
RP magnitude | 19.03 (0.05) | 18.96 | 18.96 | ||||
Pan g magnitude | 20.44 (0.02) | ||||||
Pan r magnitude | 19.72 (0.007) | ||||||
Pan i magnitude | 19.36 (0.006) | ||||||
Pan z magnitude | 19.15 (0.05) | ||||||
Pan y magnitude | 19.07 (0.06) | ||||||
E(B-V) | 0.002 |
* 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.