All names: Gaia DR2 2378136349711759232, WDJ231544.23-283333.98, WDJ231544.23-283333.99, Gaia EDR3 2378136349711759232, Gaia DR3 2378136349711759232
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
---|---|---|---|---|---|---|---|---|
Right ascension | 23 15 44.17 (0.3) | 23 15 44.17 | 23 15 44.17 | 23 15 44.23 (0.3) | 23 15 44.17 | |||
Declination | -28 33 35.46 (0.4) | -28 33 35.42 | -28 33 35.46 | -28 33 34.01 (0.4) | -28 33 35.42 | |||
Spectral type | DA: | DA | ||||||
Effective temperature | [K] | 4634.0 (160) | ||||||
log(g) | [cgs] | 7.60 (0.1) | ||||||
Mass | [M☉] | 0.365 (0.08) | ||||||
log(Luminosity) | [L☉] | |||||||
Cooling age | [Gyr] | |||||||
log(H/He) | ||||||||
log(C/He) | ||||||||
log(Ca/He) | ||||||||
log(Ca/H) | ||||||||
Parallax | [mas] | 10.27 (0.4) | 10.79 (0.6) | 10.27 | 10.27 (0.4) | 10.79 (0.6) | ||
Distance | [pc] | 97.38 (4) | 92.71 (5) | 97.38 | 97.38 (4) | 92.71 (5) | ||
Composition | ||||||||
Proper motion (right ascension) | [mas/yr] | -51.63429297 (0.4) | -49.58772642 (1) | -51.634 (0.4) | -49.58772642 | |||
Proper motion (declination) | [mas/yr] | -91.14227561 (0.4) | -92.24985638 (1) | -91.142 (0.4) | -92.24985638 | |||
Variability | ||||||||
Magnetic | ||||||||
Bd | [MG] | |||||||
Infrared excess (disk) | ||||||||
Binarity | ||||||||
B magnitude | ||||||||
V magnitude | ||||||||
R magnitude | ||||||||
I magnitude | ||||||||
J magnitude | ||||||||
H magnitude | ||||||||
K magnitude | ||||||||
u magnitude | ||||||||
g magnitude | ||||||||
r magnitude | ||||||||
i magnitude | ||||||||
z magnitude | ||||||||
G magnitude | 19.69 (0.06) | 19.73 | 19.69 | 19.69 (0.005) | 19.73 | |||
BP magnitude | 20.41 (0.06) | 20.11 | 20.11 | |||||
RP magnitude | 19.00 (0.04) | 19.07 | 19.07 | |||||
Pan g magnitude | 20.25 (0.007) | |||||||
Pan r magnitude | 19.64 (0.01) | |||||||
Pan i magnitude | 19.38 (0.009) | |||||||
Pan z magnitude | 19.33 (0.03) | |||||||
Pan y magnitude | 19.22 (0.02) | |||||||
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.