All names: Gaia DR2 4683172420470864256, 2MASS J03553188-5611282, SCR J0355-5611, WDJ035531.89-561128.32, Gaia DR3 4683172420470864256, LEP0355-5611, TIC 197909428, WISE J035532.03-561125.7, 035531.89-561128.32, WDJ035531.89-561128.31, Gaia EDR3 4683172420470864256
| Parameter | Unit | Gaia EDR3 | O'Brien et al. 2024 | O'Brien et al. 2022 | Subasavage et al. 2022 | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 03 55 32.16 (0.05) | 03 55 32.15 | 03 55 32.16 | 03 55 31.89 (0.05) | 03 55 32.15 | |||||
| Declination | -56 11 24.41 (0.05) | -56 11 24.54 | -56 11 24.41 | -56 11 28.31 (0.05) | -56 11 24.54 | |||||
| Spectral type | DAH | DAH | DAH | DA | DAH | |||||
| Effective temperature | [K] | 5771.0 (50) | 5770.0 (50) | 5639.0 (104) | 5821.0 (35) | |||||
| log(g) | [cgs] | 8.19 (0.03) | 8.19 (0.03) | 7.98 (0.05) | 8.21 (0.01) | |||||
| Mass | [M☉] | 0.707 (0.02) | 0.573 (0.04) | 0.722 (0.01) | ||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | |||||||||
| 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] | 30.35 (0.05) | 30.35 (0.05) | 30.35 (0.05) | 30.29 (0.06) | 30.29 (0.06) | 30.35 | 30.35 (0.05) | 30.29 (0.06) | |
| Distance | [pc] | 32.95 (0.05) | 32.95 (0.05) | 32.95 (0.05) | 33.01 (0.06) | 33.01 (0.06) | 32.95 | 32.95 (0.05) | 33.01 (0.06) | |
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | 144.5301674 (0.06) | 144.4888442 (0.1) | 144.53 (0.06) | 144.4888442 | |||||
| Proper motion (declination) | [mas/yr] | 243.4960544 (0.07) | 243.9537768 (0.1) | 243.496 (0.07) | 243.9537768 | |||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | 17.65 | 17.37 | ||||||||
| V magnitude | 17.09 | |||||||||
| R magnitude | 16.66 | 16.47 | ||||||||
| I magnitude | 16.13 | 16.11 | ||||||||
| J magnitude | 16.05 | 16.05 (0.1) | ||||||||
| H magnitude | 15.54 | 15.54 (0.1) | ||||||||
| K magnitude | 15.44 | |||||||||
| u magnitude | ||||||||||
| g magnitude | ||||||||||
| r magnitude | ||||||||||
| i magnitude | ||||||||||
| z magnitude | ||||||||||
| G magnitude | 17.05 (0.005) | 17.06 | 17.05 | 17.05 (0.003) | 17.06 | |||||
| BP magnitude | 17.38 (0.005) | 17.39 | 17.39 | |||||||
| RP magnitude | 16.56 (0.005) | 16.55 | 16.55 | |||||||
| Pan g magnitude | ||||||||||
| Pan r magnitude | ||||||||||
| Pan i magnitude | ||||||||||
| Pan z magnitude | ||||||||||
| Pan y magnitude | ||||||||||
| E(B-V) | 0.000 | |||||||||
* 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.