SDSS J135144.13+124255.8
All names: Gaia EDR3 3728504574726821632, SDSS J135144.13+124255.87, SDSS J135144.13+124255.8, Gaia DR2 3728504574726821632, Gaia DR3 3728504574726821632, SDSSJ135144.13+124255.8, SDSS J135144.12+124255.8
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR10 | Geier 2020 | MWDD H | Gaia DR2 | Stilism | Kepler et al. 2015 | Simbad | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 13 51 44.13 (0.2) | 13 51 44.13 | 13 51 44.13 | 13 51 44.13 (0.3) | 13 51 44.13 (0.2) | ||||||
| Declination | 12 42 55.82 (0.2) | 12 42 55.88 | 12 42 55.80 | 12 42 55.82 (0.2) | 12 42 55.87 (0.2) | ||||||
| Spectral type | sdO | He-sdO | He-sdO | DAB | sdO | ||||||
| Effective temperature | [K] | 27515.0 | 49950.0 (495) | ||||||||
| log(g) | [cgs] | 6.71 | 7.04 (0.05) | ||||||||
| Mass | [M☉] | 0.261 | |||||||||
| log(Luminosity) | [L☉] | ||||||||||
| Cooling age | [Gyr] | ||||||||||
| log(H/He) | |||||||||||
| log(C/He) | |||||||||||
| log(Ca/He) | |||||||||||
| log(Ca/H) | |||||||||||
| Parallax | [mas] | 0.45 (0.3) | 0.51 (0.4) | 0.51 (0.4) | 0.45 (0.3) | ||||||
| Distance | [pc] | 2234.11 (1432) | 1954.65 (1354) | 1954.50 (1354) | 2234.14 (1432) | ||||||
| Composition | |||||||||||
| Proper motion (right ascension) | [mas/yr] | -4.306070671 (0.3) | -5.105 (0.7) | -5.105138963 (0.7) | -4.306 (0.3) | ||||||
| Proper motion (declination) | [mas/yr] | -3.479688898 (0.2) | -3.708 (0.5) | -3.70835434 (0.5) | -3.48 (0.2) | ||||||
| Variability | |||||||||||
| Magnetic | |||||||||||
| Bd | [MG] | ||||||||||
| Infrared excess (disk) | |||||||||||
| Binarity | |||||||||||
| B magnitude | |||||||||||
| V magnitude | |||||||||||
| R magnitude | |||||||||||
| I magnitude | |||||||||||
| J magnitude | |||||||||||
| H magnitude | |||||||||||
| K magnitude | |||||||||||
| u magnitude | 18.71 (0.02) | 18.71 (0.02) | 18.73 (0.03) | 18.71 (0.02) | |||||||
| g magnitude | 19.13 (0.01) | 19.13 (0.01) | 19.15 (0.02) | 19.13 (0.01) | |||||||
| r magnitude | 19.64 (0.02) | 19.64 (0.02) | 19.65 (0.02) | 19.64 (0.02) | |||||||
| i magnitude | 20.01 (0.03) | 20.01 (0.03) | 20.03 (0.03) | 20.01 (0.03) | |||||||
| z magnitude | 20.29 (0.1) | 20.29 (0.1) | 20.29 (0.1) | 20.29 (0.1) | |||||||
| G magnitude | 19.36 (0.03) | 19.42 (0.004) | 19.42 | 19.36 (0.004) | |||||||
| BP magnitude | 19.22 (0.03) | 19.18 (0.03) | 19.18 | ||||||||
| RP magnitude | 19.69 (0.07) | 19.67 (0.05) | 19.67 | ||||||||
| Pan g magnitude | 19.18 (0.01) | 19.18 (0.01) | |||||||||
| Pan r magnitude | 19.61 (0.01) | 19.61 (0.01) | |||||||||
| Pan i magnitude | 20.00 (0.02) | 20.00 (0.02) | |||||||||
| Pan z magnitude | 20.26 (0.03) | 20.26 (0.03) | |||||||||
| Pan y magnitude | 19.96 (0.2) | 19.96 (0.2) | |||||||||
| E(B-V) | 0.026 | ||||||||||
* 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
