Gaia DR2 3129655296079487872
All names: Gaia DR3 3129655296079487872, TIC 237807615, Gaia EDR3 3129655296079487872, WDJ065729.40+055047.87, Gaia DR2 3129655296079487872, SDSS J065729.33+055047.5, 2MASS J06572938+0550479, J0657+0550, WDJ065729.4+055047.87
| 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 | 06 57 29.29 (0.08) | 06 57 29.29 (0.1) | 06 57 29.29 | 06 57 29.29 | 06 57 29.40 (0.08) | 06 57 29.29 | ||||||||
| Declination | 05 50 47.42 (0.09) | 05 50 47.43 (0.1) | 05 50 47.43 | 05 50 47.42 | 05 50 47.87 (0.09) | 05 50 47.43 | ||||||||
| Spectral type | DC | DC | DC | DC | DA | DC | ||||||||
| Effective temperature | [K] | 6010.0 (70) | 5855.0 (24) | 6018.5 (61) | 6020.0 (60) | 6246.0 | 5990.0 | 6143.0 (57) | ||||||
| log(g) | [cgs] | 8.19 (0.04) | 8.13 (0.01) | 8.21 (0.03) | 8.21 (0.04) | 8.32 | 8.19 | 8.27 (0.02) | ||||||
| Mass | [M☉] | 0.691 (0.03) | 0.656 (0.009) | 0.796 | 0.692 | 0.761 (0.02) | ||||||||
| log(Luminosity) | [L☉] | |||||||||||||
| Cooling age | [Gyr] | 4.0700 | 4.0340 | 4.0420 | ||||||||||
| log(H/He) | ||||||||||||||
| log(C/He) | ||||||||||||||
| 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] | 25.64 (0.1) | 25.64 (0.1) | 25.74 (0.1) | 25.74 (0.1) | 25.74 (0.1) | 25.64 | 25.64 (0.1) | 25.74 (0.1) | |||||
| Distance | [pc] | 39.00 (0.2) | 39.00 (0.2) | 38.85 (0.2) | 38.85 (0.2) | 38.85 (0.2) | 39.00 | 39.00 (0.2) | 38.85 (0.2) | |||||
| Composition | He | He | ||||||||||||
| Proper motion (right ascension) | [mas/yr] | -104.6562174 (0.1) | -104.8058226 (0.2) | -104.656 (0.1) | -104.8058226 | |||||||||
| Proper motion (declination) | [mas/yr] | -28.13244435 (0.09) | -28.21450066 (0.2) | -28.132 (0.09) | -28.21450066 | |||||||||
| Variability | ||||||||||||||
| Magnetic | ||||||||||||||
| Bd | [MG] | |||||||||||||
| Infrared excess (disk) | ||||||||||||||
| Binarity | ||||||||||||||
| B magnitude | ||||||||||||||
| V magnitude | ||||||||||||||
| R magnitude | ||||||||||||||
| I magnitude | ||||||||||||||
| J magnitude | 16.39 (0.1) | 16.39 (0.1) | ||||||||||||
| H magnitude | 15.98 (0.2) | 15.98 (0.2) | ||||||||||||
| K magnitude | ||||||||||||||
| u magnitude | 18.50 (0.02) | 18.51 (0.02) | 18.51 (0.02) | |||||||||||
| g magnitude | 17.59 (0.005) | 17.59 (0.005) | ||||||||||||
| r magnitude | 17.30 (0.005) | 17.30 (0.005) | ||||||||||||
| i magnitude | 17.18 (0.006) | 17.18 (0.006) | ||||||||||||
| z magnitude | 17.19 (0.01) | 17.19 (0.01) | ||||||||||||
| G magnitude | 17.27 (0.007) | 17.28 | 17.28 | 17.27 | 17.27 (0.003) | 17.28 | ||||||||
| BP magnitude | 17.55 (0.007) | 17.55 | 17.55 | |||||||||||
| RP magnitude | 16.83 (0.007) | 16.84 | 16.84 | |||||||||||
| Pan g magnitude | 17.56 (0.005) | 17.56 (0.005) | ||||||||||||
| Pan r magnitude | 17.28 (0.005) | 17.28 (0.005) | ||||||||||||
| Pan i magnitude | 17.19 (0.003) | 17.19 (0.003) | ||||||||||||
| Pan z magnitude | 17.18 (0.006) | 17.18 (0.005) | ||||||||||||
| Pan y magnitude | 17.21 (0.02) | 17.21 (0.02) | ||||||||||||
| E(B-V) | 0.000 | |||||||||||||
* 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
