All names: USNO-B1.0 1293-00320425, EGGR 580, Gaia EDR3 2100304020669107328, Gaia DR2 2100304020669107328, TIC 120424803, 1858+393, 2MASS J19001730+3922356, Gaia DR3 2100304020669107328, SDSS J190017.32+392234.0, WD 1858+393, WD 1858+39, NLTT 47312, WDJ190017.30+392235.25, UCAC2 45529620, J1900+3922, KIC 4242459, G205-52, LSPM J1900+3922, G 205-52, PM J19002+3922
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Caron et al. 2023 | Leggett et al. 2018 | MWDD H | Gaia DR2 | Stilism | Gianninas et al. 2011 | Farihi et al. 2008 | Kilic et al. 2006 | Zuckerman et al. 2003 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 19 00 17.35 (0.02) | 19 00 17.35 (0.03) | 19 00 17.35 | 19 00 17.30 (0.02) | 19 00 17.35 | 19 00 16.85 | ||||||||||
| Declination | 39 22 31.51 (0.02) | 39 22 31.62 (0.03) | 39 22 31.51 | 39 22 35.25 (0.02) | 39 22 31.62 | 39 22 41.16 | ||||||||||
| Spectral type | DA | DA5.4 | DA | DA | DAZ | DAZ | DA | DA5.3 | DA6 | |||||||
| Effective temperature | [K] | 9434.0 (28) | 9380.0 (255) | 9279.0 | 9530.0 (137) | 9470.0 | 9470.0 | 9470.0 | 9328.0 (46) | |||||||
| log(g) | [cgs] | 8.01 (0.005) | 7.93 (0.04) | 7.98 | 8.26 (0.05) | 8.00 | 8.00 | 7.99 (0.009) | ||||||||
| Mass | [M☉] | 0.606 (0.004) | 0.557 (0.04) | 0.584 | 0.76 (0.03) | 0.591 (0.007) | ||||||||||
| log(Luminosity) | [L☉] | |||||||||||||||
| Cooling age | [Gyr] | 0.7500 | 0.6480 (0.06) | 0.7086 | ||||||||||||
| log(H/He) | ||||||||||||||||
| log(C/He) | ||||||||||||||||
| log(Ca/He) | ||||||||||||||||
| log(Ca/H) | -7.84 | -7.8 | -7.844 | |||||||||||||
| log(C/H) | ||||||||||||||||
| log(N/H) | ||||||||||||||||
| log(O/H) | ||||||||||||||||
| log(Na/H) | ||||||||||||||||
| log(Mg/H) | -6.8 | |||||||||||||||
| 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) | -6.92 | |||||||||||||||
| log(Ni/H) | ||||||||||||||||
| Parallax | [mas] | 22.55 (0.02) | 22.51 (0.03) | 21.45 (0.4) | 22.51 (0.03) | 22.55 | 22.55 (0.02) | 22.51 (0.03) | ||||||||
| Distance | [pc] | 44.34 (0.05) | 44.42 (0.06) | 46.62 (1) | 44.43 (0.06) | 37.00 | 44.34 | 44.34 (0.05) | 44.43 (0.06) | |||||||
| Composition | H | H | H | H | H | |||||||||||
| Proper motion (right ascension) | [mas/yr] | 42.19374873 (0.03) | 42.21710657 (0.06) | 42.194 (0.03) | 42.21710657 | |||||||||||
| Proper motion (declination) | [mas/yr] | -233.9700224 (0.03) | -233.994989 (0.06) | -233.97 (0.03) | -233.994989 | |||||||||||
| Variability | ||||||||||||||||
| Magnetic | ||||||||||||||||
| Bd | [MG] | |||||||||||||||
| Infrared excess (disk) | ||||||||||||||||
| Binarity | ||||||||||||||||
| B magnitude | 16.70 | |||||||||||||||
| V magnitude | 15.63 | |||||||||||||||
| R magnitude | 15.60 | |||||||||||||||
| I magnitude | ||||||||||||||||
| J magnitude | 15.47 (0.007) | 15.43 | 15.53 (0.05) | |||||||||||||
| H magnitude | 15.44 (0.09) | 15.36 | 15.44 (0.09) | |||||||||||||
| K magnitude | 15.25 (0.1) | 15.43 | 15.25 (0.1) | |||||||||||||
| u magnitude | 16.07 (0.006) | 16.09 (0.02) | 16.07 (0.006) | |||||||||||||
| g magnitude | 15.64 (0.01) | 15.64 (0.003) | ||||||||||||||
| r magnitude | 15.68 (0.008) | 15.68 (0.004) | ||||||||||||||
| i magnitude | 15.78 (0.01) | 15.78 (0.004) | ||||||||||||||
| z magnitude | 15.92 (0.02) | 15.94 (0.007) | ||||||||||||||
| G magnitude | 15.62 (0.002) | 15.64 | 15.62 | 15.62 (0.003) | 15.64 | |||||||||||
| BP magnitude | 15.70 (0.002) | 15.69 | 15.69 | |||||||||||||
| RP magnitude | 15.48 (0.003) | 15.49 | 15.49 | |||||||||||||
| Pan g magnitude | 15.65 (0.003) | 15.65 (0.003) | ||||||||||||||
| Pan r magnitude | 15.71 (0.004) | 15.71 (0.003) | ||||||||||||||
| Pan i magnitude | 15.81 (0.002) | 15.81 (0.002) | ||||||||||||||
| Pan z magnitude | 15.94 (0.001) | 15.94 (0.001) | ||||||||||||||
| Pan y magnitude | 16.04 (0.003) | 16.04 (0.003) | ||||||||||||||
| E(B-V) | 0.005 | |||||||||||||||
* 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.