All names: SDSS J155155.26+082431.8, GALEX J155155.2+082432, Gaia DR2 4454432667131057792, J1551+0824, Gaia DR3 4454432667131057792, SDSS J155155.26+082431.7, Gaia EDR3 4454432667131057792, WDJ155155.25+082431.94
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Caron et al. 2023 | Coutu et al. 2019 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | Kleinman et al. 2013 | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 15 51 55.27 (0.1) | 15 51 55.26 | 15 51 55.25 | 15 51 55.27 (0.1) | 15 51 55.27 | 15 51 55.25 (0.1) | 15 51 55.27 | 15 51 55.26 | |||||||
| Declination | 08 24 30.92 (0.08) | 08 24 31.70 | 08 24 31.94 | 08 24 30.95 (0.1) | 08 24 30.92 | 08 24 31.94 (0.08) | 08 24 30.95 | 08 24 31.76 | |||||||
| Spectral type | DQ | DQ | DC | DQ | DQ | DQ | |||||||||
| Effective temperature | [K] | 6765.0 (36) | 6768.0 (109) | 7276.0 | 7006.0 | 6628.0 (127) | 10080.0 (2) | ||||||||
| log(g) | [cgs] | 7.97 (0.01) | 7.98 | 8.20 | 8.09 | 7.95 (0.03) | 9.87 (0.2) | ||||||||
| Mass | [M☉] | 0.557 (0.01) | 0.5604 | 0.717 | 0.632 | 0.546 (0.03) | |||||||||
| log(Luminosity) | [L☉] | ||||||||||||||
| Cooling age | [Gyr] | 1.7100 | 1.6300 | 1.8970 | 1.8190 | ||||||||||
| log(H/He) | |||||||||||||||
| log(C/He) | -6.3 | -6.2803 (0.03) | |||||||||||||
| log(Ca/He) | |||||||||||||||
| log(Ca/H) | |||||||||||||||
| log(N/He) | |||||||||||||||
| log(O/He) | |||||||||||||||
| log(Na/He) | |||||||||||||||
| log(Mg/He) | |||||||||||||||
| log(Al/He) | |||||||||||||||
| log(Si/He) | |||||||||||||||
| log(P/He) | |||||||||||||||
| log(S/He) | |||||||||||||||
| log(Cl/He) | |||||||||||||||
| log(Sc/He) | |||||||||||||||
| log(Ti/He) | |||||||||||||||
| log(V/He) | |||||||||||||||
| log(Cr/He) | |||||||||||||||
| log(Mn/He) | |||||||||||||||
| log(Fe/He) | |||||||||||||||
| log(Co/He) | |||||||||||||||
| log(Ni/He) | |||||||||||||||
| log(Cu/He) | |||||||||||||||
| log(Zn/He) | |||||||||||||||
| log(Ga/He) | |||||||||||||||
| log(Ge/He) | |||||||||||||||
| log(Sr/He) | |||||||||||||||
| Parallax | [mas] | 13.99 (0.1) | 13.90 (0.1) | 13.90 | 13.90 (0.1) | 13.99 | 13.99 (0.1) | 13.90 (0.1) | |||||||
| Distance | [pc] | 71.46 (0.6) | 71.94 (0.7) | 71.94 (0.7) | 71.94 (0.7) | 71.46 | 71.46 (0.6) | 71.94 (0.7) | |||||||
| Composition | He | He | |||||||||||||
| Proper motion (right ascension) | [mas/yr] | 14.40899095 (0.1) | 14.40519369 (0.3) | 14.409 (0.1) | 14.40519369 | ||||||||||
| Proper motion (declination) | [mas/yr] | -63.5744046 (0.1) | -63.43375918 (0.2) | -63.574 (0.1) | -63.43375918 | ||||||||||
| Variability | |||||||||||||||
| Magnetic | |||||||||||||||
| Bd | [MG] | ||||||||||||||
| Infrared excess (disk) | |||||||||||||||
| Binarity | |||||||||||||||
| B magnitude | |||||||||||||||
| V magnitude | |||||||||||||||
| R magnitude | |||||||||||||||
| I magnitude | |||||||||||||||
| J magnitude | 17.37 (0.02) | 17.37 (0.02) | |||||||||||||
| H magnitude | 17.22 (0.05) | 17.22 (0.06) | |||||||||||||
| K magnitude | 17.17 (0.07) | 17.17 (0.07) | |||||||||||||
| u magnitude | 18.53 (0.02) | 18.50 (0.02) | 18.53 (0.02) | 18.50 (0.02) | 18.52 (0.02) | ||||||||||
| g magnitude | 18.03 (0.006) | 18.03 (0.006) | 18.04 (0.006) | 18.07 (0.02) | |||||||||||
| r magnitude | 17.89 (0.006) | 17.89 (0.006) | 17.87 (0.006) | 17.89 (0.01) | |||||||||||
| i magnitude | 17.86 (0.008) | 17.86 (0.008) | 17.85 (0.007) | 17.86 (0.01) | |||||||||||
| z magnitude | 17.96 (0.02) | 17.96 (0.02) | 17.93 (0.02) | 17.94 (0.02) | |||||||||||
| G magnitude | 17.85 (0.01) | 17.87 | 17.85 | 17.85 (0.003) | 17.87 | ||||||||||
| BP magnitude | 18.05 (0.01) | 18.06 | 18.06 | ||||||||||||
| RP magnitude | 17.55 (0.01) | 17.55 | 17.55 | ||||||||||||
| Pan g magnitude | 18.03 (0.009) | 18.03 (0.01) | |||||||||||||
| Pan r magnitude | 17.88 (0.004) | 17.88 (0.004) | |||||||||||||
| Pan i magnitude | 17.88 (0.004) | 17.88 (0.004) | |||||||||||||
| Pan z magnitude | 17.94 (0.008) | 17.94 (0.005) | |||||||||||||
| Pan y magnitude | 17.98 (0.008) | 17.98 (0.008) | |||||||||||||
| E(B-V) | 0.004 | ||||||||||||||
* 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.