Gaia DR2 2064838031864808832
All names: J2035+4054, Gaia DR2 2064838031864808832, WDJ203550.05+405438.30, Gaia DR3 2064838031864808832, Gaia EDR3 2064838031864808832, SDSS J203550.07+405438.6, WDJ203550.05+405438.31
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | Bergeron et al. 2022 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 20 35 50.17 (0.2) | 20 35 50.17 | 20 35 50.17 | 20 35 50.05 (0.2) | 20 35 50.17 | |||||||
| Declination | 40 54 39.46 (0.2) | 40 54 39.43 | 40 54 39.46 | 40 54 38.30 (0.2) | 40 54 39.43 | |||||||
| Spectral type | IRfaint | DC | DC: | DC | ||||||||
| Effective temperature | [K] | 3021.0 (65) | 3021.0 (65) | 4804.0 | 4565.0 | 4724.0 (110) | ||||||
| log(g) | [cgs] | 7.23 (0.03) | 8.48 | 8.34 | 8.39 (0.05) | |||||||
| Mass | [M☉] | 0.24 (0.009) | 0.24 (0.009) | 0.894 | 0.787 | 0.837 (0.04) | ||||||
| log(Luminosity) | [L☉] | |||||||||||
| Cooling age | [Gyr] | 8.9720 | 9.1290 | 7.7530 | ||||||||
| log(H/He) | -0.27 | -0.27 | ||||||||||
| log(C/He) | ||||||||||||
| log(Ca/He) | ||||||||||||
| log(Ca/H) | ||||||||||||
| Parallax | [mas] | 20.03 (0.2) | 19.75 (0.3) | 20.03 | 20.03 (0.2) | 19.75 (0.3) | ||||||
| Distance | [pc] | 49.93 (0.6) | 50.64 (0.7) | 49.93 | 49.93 (0.6) | 50.64 (0.7) | ||||||
| Composition | ||||||||||||
| Proper motion (right ascension) | [mas/yr] | 88.76109443 (0.2) | 88.4478963 (0.5) | 88.761 (0.2) | 88.4478963 | |||||||
| Proper motion (declination) | [mas/yr] | 72.42133433 (0.2) | 72.36829696 (0.5) | 72.421 (0.2) | 72.36829696 | |||||||
| Variability | ||||||||||||
| Magnetic | ||||||||||||
| Bd | [MG] | |||||||||||
| Infrared excess (disk) | ||||||||||||
| Binarity | ||||||||||||
| B magnitude | ||||||||||||
| V magnitude | ||||||||||||
| R magnitude | ||||||||||||
| I magnitude | ||||||||||||
| J magnitude | ||||||||||||
| H magnitude | ||||||||||||
| K magnitude | ||||||||||||
| u magnitude | 22.80 (0.4) | 22.87 (0.5) | ||||||||||
| g magnitude | 20.27 (0.02) | 20.21 (0.02) | ||||||||||
| r magnitude | 18.87 (0.01) | 18.91 (0.01) | ||||||||||
| i magnitude | 18.64 (0.01) | 18.64 (0.01) | ||||||||||
| z magnitude | 19.05 (0.05) | 19.08 (0.07) | ||||||||||
| G magnitude | 19.08 (0.05) | 19.12 | 19.08 | 19.08 (0.004) | 19.12 | |||||||
| BP magnitude | 19.83 (0.05) | 19.72 | 19.72 | |||||||||
| RP magnitude | 18.42 (0.03) | 18.40 | 18.40 | |||||||||
| Pan g magnitude | 20.05 (0.02) | |||||||||||
| Pan r magnitude | 18.92 (0.01) | |||||||||||
| Pan i magnitude | 18.67 (0.01) | |||||||||||
| Pan z magnitude | 18.91 (0.04) | |||||||||||
| Pan y magnitude | 19.33 (0.07) | |||||||||||
| E(B-V) | 0.004 | |||||||||||
* Constant surface field
Special notes:
Spectra
Controls
Normalize at:
Normalize by mean flux
Range:
x:
to
y:
to
Spectra available:
Spectra without link are available upon request
Absorption lines
Photometric filters
BVRI
ugriz
Photometric fit
