All names: WISE J114110.90-372924.1, Gaia DR3 5385898889087248256, DENIS J114110.8-372924, WDJ114110.85-372923.97, TIC 454013177, 2MASS J11411085-3729240, Gaia EDR3 5385898889087248256, WDJ114110.85-372923.98, Gaia DR2 5385898889087248256, WISEA J114110.88-372924.2
| Parameter | Unit | Gaia EDR3 | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|
| Right ascension | 11 41 10.72 (0.04) | 11 41 10.72 | 11 41 10.72 | 11 41 10.85 (0.04) | 11 41 10.72 | ||
| Declination | -37 29 23.85 (0.03) | -37 29 23.86 | -37 29 23.85 | -37 29 23.98 (0.03) | -37 29 23.86 | ||
| Spectral type | DA | DA | |||||
| Effective temperature | [K] | 17828.0 (240) | |||||
| log(g) | [cgs] | 8.54 (0.01) | |||||
| Mass | [M☉] | 0.954 (0.009) | |||||
| log(Luminosity) | [L☉] | ||||||
| Cooling age | [Gyr] | ||||||
| log(H/He) | |||||||
| log(C/He) | |||||||
| log(Ca/He) | |||||||
| log(Ca/H) | |||||||
| Parallax | [mas] | 12.62 (0.05) | 12.63 (0.08) | 12.62 | 12.62 (0.05) | 12.63 (0.08) | |
| Distance | [pc] | 79.25 (0.3) | 79.16 (0.5) | 79.25 | 79.25 (0.3) | 79.16 (0.5) | |
| Composition | |||||||
| Proper motion (right ascension) | [mas/yr] | -99.24802379 (0.06) | -99.39841633 (0.1) | -99.248 (0.06) | -99.39841633 | ||
| Proper motion (declination) | [mas/yr] | 7.85080936 (0.04) | 7.777069719 (0.07) | 7.851 (0.04) | 7.777069719 | ||
| Variability | |||||||
| Magnetic | |||||||
| Bd | [MG] | ||||||
| Infrared excess (disk) | |||||||
| Binarity | |||||||
| B magnitude | |||||||
| V magnitude | |||||||
| R magnitude | |||||||
| I magnitude | 16.51 (0.07) | ||||||
| J magnitude | 16.55 (0.2) | ||||||
| H magnitude | |||||||
| K magnitude | |||||||
| u magnitude | |||||||
| g magnitude | |||||||
| r magnitude | |||||||
| i magnitude | |||||||
| z magnitude | |||||||
| G magnitude | 16.36 (0.003) | 16.38 | 16.36 | 16.36 (0.003) | 16.38 | ||
| BP magnitude | 16.30 (0.003) | 16.28 | 16.28 | ||||
| RP magnitude | 16.52 (0.004) | 16.52 | 16.52 | ||||
| Pan g magnitude | |||||||
| Pan r magnitude | |||||||
| Pan i magnitude | |||||||
| Pan z magnitude | |||||||
| Pan y magnitude | |||||||
| E(B-V) | 0.003 | ||||||
* 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.