All names: Gaia DR2 3549471753507182592, SDSS J105638.59-225254.3, WD 1054-226, TIC 415714190, LP 849-31, Gaia DR3 3549471753507182592, GALEX J105638.5-225253, WDJ105638.63-225256.08, LEHPM 2-1372, PSO J164.1606-22.8810, J1056-2252, NLTT 25792, 2MASS J10563864-2252564, Gaia EDR3 3549471753507182592, EC 10542-2236
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | O'Brien et al. 2024 | Caron et al. 2023 | Blouin et al. 2019 | MWDD H | Gaia DR2 | Stilism | Gianninas et al. 2011 | Subasavage et al. 2007 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 10 56 38.54 (0.04) | 10 56 38.54 (0.05) | 10 56 38.64 | 10 56 38.54 | 10 56 38.63 (0.04) | 10 56 38.54 | 10 56 37.97 | ||||||||
| Declination | -22 52 51.31 (0.04) | -22 52 51.46 (0.05) | -22 52 55.90 | -22 52 51.31 | -22 52 56.08 (0.04) | -22 52 51.46 | -22 52 56.64 | ||||||||
| Spectral type | DAZ | DA | DA | DA | DA | DA6.0 | DA | DAZ6.4 | DA6.1 | ||||||
| Effective temperature | [K] | 7836.0 (112) | 7783.0 (35) | 7690.0 (70) | 7570.0 | 7910.0 (118) | 8266.0 (324) | 7641.0 (53) | |||||||
| log(g) | [cgs] | 8.10 (0.04) | 8.08 (0.007) | 8.07 (0.02) | 8.03 | 8.05 (0.08) | 8.05 (0.01) | ||||||||
| Mass | [M☉] | 0.655 (0.02) | 0.645 (0.007) | 0.636 (0.01) | 0.61 | 0.62 (0.05) | 0.622 (0.01) | ||||||||
| log(Luminosity) | [L☉] | ||||||||||||||
| Cooling age | [Gyr] | 1.3500 | 1.3120 (0.05) | 1.2890 | |||||||||||
| 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] | 27.65 (0.05) | 27.65 (0.05) | 27.62 (0.07) | 27.62 (0.07) | 27.62 (0.07) | 27.65 | 27.65 (0.05) | 27.62 (0.07) | ||||||
| Distance | [pc] | 36.16 (0.07) | 36.17 (0.07) | 36.21 (0.09) | 36.20 (0.09) | 36.20 (0.09) | 37.00 | 41.00 | 36.16 | 36.16 (0.07) | 36.20 (0.09) | ||||
| Composition | H | H | H | H | H | ||||||||||
| Proper motion (right ascension) | [mas/yr] | -78.86490054 (0.05) | -78.91864499 (0.1) | -78.865 (0.05) | -78.91864499 | ||||||||||
| Proper motion (declination) | [mas/yr] | 298.0189658 (0.05) | 297.9480687 (0.09) | 298.019 (0.05) | 297.9480687 | ||||||||||
| Variability | |||||||||||||||
| Magnetic | |||||||||||||||
| Bd | [MG] | ||||||||||||||
| Infrared excess (disk) | |||||||||||||||
| Binarity | |||||||||||||||
| B magnitude | 16.57 | ||||||||||||||
| V magnitude | 16.00 | ||||||||||||||
| R magnitude | 15.82 | ||||||||||||||
| I magnitude | 15.62 | ||||||||||||||
| J magnitude | 15.44 (0.005) | 15.52 (0.05) | 15.52 (0.05) | 15.52 (0.05) | |||||||||||
| H magnitude | 15.40 (0.1) | 15.40 (0.1) | 15.40 (0.1) | 15.40 (0.1) | |||||||||||
| K magnitude | 15.31 (0.02) | 15.94 (0.3) | 15.94 (0.3) | 15.94 (0.3) | |||||||||||
| u magnitude | 16.55 (0.03) | 16.55 (0.01) | |||||||||||||
| g magnitude | 16.09 (0.003) | ||||||||||||||
| r magnitude | 16.02 (0.003) | ||||||||||||||
| i magnitude | 16.01 (0.007) | ||||||||||||||
| z magnitude | 16.09 (0.005) | ||||||||||||||
| G magnitude | 15.96 (0.006) | 15.97 | 15.96 | 15.96 (0.003) | 15.97 | ||||||||||
| BP magnitude | 16.10 (0.006) | 16.10 | 16.10 | ||||||||||||
| RP magnitude | 15.70 (0.005) | 15.71 | 15.71 | ||||||||||||
| Pan g magnitude | 16.13 (0) | 16.13 (0) | 16.09 (0.003) | ||||||||||||
| Pan r magnitude | 15.98 (0.0008) | 15.98 (0.002) | 16.02 (0.003) | ||||||||||||
| Pan i magnitude | 16.03 (0.004) | 16.03 (0.004) | 16.01 (0.007) | ||||||||||||
| Pan z magnitude | 16.11 (0.007) | 16.11 (0.007) | 16.09 (0.005) | ||||||||||||
| Pan y magnitude | 16.14 (0.005) | 16.14 (0.005) | 16.14 (0.01) | ||||||||||||
| E(B-V) | 0.001 | ||||||||||||||
* 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.