WD 0742+432
All names: Gaia DR2 924345239195423232, SDSS J074532.47+430530.3, SDSS J074532.46+430530.5, Gaia EDR3 924345239195423232, Gaia DR3 924345239195423232, SDSS J074532.48+430530.5, WD 0742+432, SDSS J074532.46+430530.3, SDSS J074532.46+430530.4, GALEX J074532.4+430530, SDSS J074532.47+430530.5
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | MWDD H | Gaia DR2 | Stilism | sdss-wdms.org (29/04/2016) | Tremblay et al. 2011 | Vincent et al. 2024 | Simbad | Eisenstein et al. 2006 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 | Kleinman et al. 2004 | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 07 45 32.48 (0.1) | 07 45 32.47 | 07 45 32.48 (0.2) | 07 45 32.48 | 07 45 32.48 | 07 45 32.47 (0.1) | 07 45 32.47 | 07 45 32.06 | 07 45 32.48 | 07 45 32.48 | ||||||
| Declination | 43 05 30.22 (0.1) | 43 05 30.55 | 43 05 30.23 (0.1) | 43 05 30.52 | 43 05 30.22 | 43 05 30.58 (0.1) | 43 05 30.53 | 43 05 23.64 | 43 05 30.53 | 43 05 30.52 | ||||||
| Spectral type | DA+M: | DA+M: | DA | DA | DA+M | DA | DA2.1 | DA+M | DA | |||||||
| Effective temperature | [K] | 18985.0 | 23886.0 (492) | 25200.0 (390) | 23053.0 (2025) | 24277.0 (374) | 24442.0 (320) | 24502.0 (393) | ||||||||
| log(g) | [cgs] | 7.68 | 7.91 (0.07) | 7.94 (0.06) | 7.72 (0.1) | 7.92 (0.04) | 7.92 (0.04) | 7.95 (0.04) | ||||||||
| Mass | [M☉] | 0.462 | 0.58 (0.04) | 0.6 (0.03) | 0.489 (0.08) | |||||||||||
| log(Luminosity) | [L☉] | |||||||||||||||
| Cooling age | [Gyr] | 0.0524 | 0.0200 | |||||||||||||
| log(H/He) | ||||||||||||||||
| log(C/He) | ||||||||||||||||
| log(Ca/He) | ||||||||||||||||
| log(Ca/H) | ||||||||||||||||
| log(C/H) | ||||||||||||||||
| log(N/H) | ||||||||||||||||
| log(O/H) | ||||||||||||||||
| log(Na/H) | ||||||||||||||||
| log(Mg/H) | ||||||||||||||||
| 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) | ||||||||||||||||
| log(Ni/H) | ||||||||||||||||
| Parallax | [mas] | 2.17 (0.2) | 2.38 (0.2) | 2.17 | 2.17 (0.2) | |||||||||||
| Distance | [pc] | 461.57 (34) | 420.82 (36) | 1627.00 (299) | 461.57 | 461.57 (34) | ||||||||||
| Composition | H | H | ||||||||||||||
| Proper motion (right ascension) | [mas/yr] | 3.04915811 (0.2) | 3.423253283 (0.3) | 3.049 (0.2) | 1.7 | -1.0 | ||||||||||
| Proper motion (declination) | [mas/yr] | -21.99441478 (0.1) | -22.00649017 (0.3) | -21.994 (0.1) | -25.2 | -26.0 | ||||||||||
| Variability | ||||||||||||||||
| Magnetic | ||||||||||||||||
| Bd | [MG] | |||||||||||||||
| Infrared excess (disk) | ||||||||||||||||
| Binarity | WDMS | WDMS | ||||||||||||||
| B magnitude | ||||||||||||||||
| V magnitude | ||||||||||||||||
| R magnitude | ||||||||||||||||
| I magnitude | ||||||||||||||||
| J magnitude | ||||||||||||||||
| H magnitude | ||||||||||||||||
| K magnitude | ||||||||||||||||
| u magnitude | 18.25 (0.01) | 18.24 | 18.25 (0.01) | 18.24 (0.02) | 18.25 | 18.24 (0.02) | 18.25 (0.02) | |||||||||
| g magnitude | 18.34 (0.007) | 18.36 | 18.34 (0.007) | 18.36 (0.02) | 18.35 | 18.36 (0.02) | 18.35 (0.02) | |||||||||
| r magnitude | 18.70 (0.009) | 18.70 | 18.70 (0.009) | 18.70 (0.01) | 18.71 | 18.70 (0.01) | 18.71 (0.01) | |||||||||
| i magnitude | 19.00 (0.01) | 19.01 | 19.00 (0.01) | 19.01 (0.02) | 19.01 | 19.00 (0.02) | 19.01 (0.02) | |||||||||
| z magnitude | 19.30 (0.05) | 19.31 | 19.30 (0.05) | 19.31 (0.05) | 19.32 | 19.30 (0.05) | 19.32 (0.05) | |||||||||
| G magnitude | 18.53 (0.01) | 18.56 | 18.53 | 18.53 (0.003) | ||||||||||||
| BP magnitude | 18.43 (0.01) | 18.39 | ||||||||||||||
| RP magnitude | 18.71 (0.04) | 18.65 | ||||||||||||||
| Pan g magnitude | 18.37 (0.004) | |||||||||||||||
| Pan r magnitude | 18.74 (0.01) | |||||||||||||||
| Pan i magnitude | 19.05 (0.006) | |||||||||||||||
| Pan z magnitude | 19.29 (0.02) | |||||||||||||||
| Pan y magnitude | 19.46 (0.02) | |||||||||||||||
| E(B-V) | 0.032 | |||||||||||||||
* 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
