All names: NLTT 9087, LSPM J0250+0817, Gaia EDR3 20484382662003968, Gaia DR2 20484382662003968, WDJ025007.11+081753.42, Gaia DR3 20484382662003968, J0250+0817, 2MASS J02500710+0817534, WDJ02507.11+081753.42, TIC 387464389, USNO-B1.0 0982-00037977, LP 531-14
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | O'Brien et al. 2024 | Caron et al. 2023 | McCleery et al. 2020 | Tremblay et al. 2020 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 02 50 07.33 (0.1) | 02 50 07.32 (0.2) | 02 50 07.32 | 02 50 07.33 | 02 50 07.11 (0.1) | 02 50 07.32 | ||||||||
| Declination | 08 17 46.70 (0.1) | 08 17 46.91 (0.1) | 08 17 46.91 | 08 17 46.70 | 08 17 53.42 (0.1) | 08 17 46.91 | ||||||||
| Spectral type | DC | DC | DC | DC | DA | DC | ||||||||
| Effective temperature | [K] | 4623.0 (109) | 4498.0 (20) | 4329.3 (86) | 4330.0 (90) | 4511.0 | 4205.0 | 4569.0 (62) | ||||||
| log(g) | [cgs] | 7.87 (0.09) | 7.75 (0.01) | 7.65 (0.08) | 7.65 (0.08) | 7.76 | 7.51 | 7.83 (0.03) | ||||||
| Mass | [M☉] | 0.499 (0.04) | 0.434 (0.01) | 0.441 | 0.317 | 0.477 (0.03) | ||||||||
| log(Luminosity) | [L☉] | |||||||||||||
| Cooling age | [Gyr] | 5.2100 | 4.8600 | 3.5320 | ||||||||||
| 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] | 26.32 (0.1) | 26.32 (0.1) | 25.97 (0.2) | 25.97 (0.2) | 25.97 (0.2) | 26.32 | 26.32 (0.1) | 25.97 (0.2) | |||||
| Distance | [pc] | 38.00 (0.2) | 37.99 (0.2) | 38.51 (0.3) | 38.50 (0.3) | 38.50 (0.3) | 38.00 | 38.00 (0.2) | 38.50 (0.3) | |||||
| Composition | H | |||||||||||||
| Proper motion (right ascension) | [mas/yr] | 206.2047136 (0.1) | 206.4276391 (0.3) | 206.205 (0.1) | 206.4276391 | |||||||||
| Proper motion (declination) | [mas/yr] | -420.1376492 (0.1) | -420.3614387 (0.2) | -420.138 (0.1) | -420.3614387 | |||||||||
| Variability | ||||||||||||||
| Magnetic | ||||||||||||||
| Bd | [MG] | |||||||||||||
| Infrared excess (disk) | ||||||||||||||
| Binarity | ||||||||||||||
| B magnitude | 19.70 | |||||||||||||
| V magnitude | ||||||||||||||
| R magnitude | 18.50 | |||||||||||||
| I magnitude | ||||||||||||||
| J magnitude | 16.24 (0.1) | 16.24 (0.1) | ||||||||||||
| H magnitude | 16.30 (0.2) | 16.30 (0.2) | ||||||||||||
| K magnitude | ||||||||||||||
| u magnitude | ||||||||||||||
| g magnitude | ||||||||||||||
| r magnitude | ||||||||||||||
| i magnitude | ||||||||||||||
| z magnitude | ||||||||||||||
| G magnitude | 17.98 (0.03) | 18.00 | 18.00 | 17.98 | 17.98 (0.003) | 18.00 | ||||||||
| BP magnitude | 18.58 (0.03) | 18.60 | 18.60 | |||||||||||
| RP magnitude | 17.28 (0.01) | 17.25 | 17.25 | |||||||||||
| Pan g magnitude | 18.73 (0.005) | 18.75 (0.01) | ||||||||||||
| Pan r magnitude | 17.93 (0.007) | 17.94 (0.002) | ||||||||||||
| Pan i magnitude | 17.60 (0.005) | 17.61 (0.004) | ||||||||||||
| Pan z magnitude | 17.45 (0.009) | 17.48 (0.008) | ||||||||||||
| Pan y magnitude | 17.44 (0.02) | 17.42 (0.005) | ||||||||||||
| 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.