All names: SDSS J075106.52+301726.4, LAMOST J075106.48+301727.0, 2MASS J07510650+3017267, LAMOST J075106.48+301726.96, GALEX J075106.5+301727, SDSS J075106.51+301726.4, Ton 290, Gaia DR3 878975541144130688, WD 0747+304, Gaia EDR3 878975541144130688, 1RXS J075107.4+301719, LAMOST J075106.52+301726.3, TIC 4559038, Gaia DR2 878975541144130688, LAMOST J075106.47+301726.9
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | Bedard et al. 2020 | MWDD H | Gaia DR2 | Stilism | Guo et al. 2015 | Zhao et al. 2013 | Tremblay et al. 2011 | Vincent et al. 2024 | Simbad | Eisenstein et al. 2006 | White Dwarf Catalog (McCook & Sion 1999) | Kleinman et al. 2013 | Vincent et al. 2023 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 07 51 06.53 (0.05) | 07 51 06.52 | 07 51 06.53 (0.08) | 07 51 06.47 | 07 51 06.53 | 07 51 06.51 (0.05) | 07 51 06.51 | 07 51 06.48 | 07 51 06.52 | ||||||||
Declination | 30 17 26.30 (0.04) | 30 17 26.49 | 30 17 26.30 (0.05) | 30 17 26.96 | 30 17 26.30 | 30 17 26.48 (0.04) | 30 17 26.42 | 30 17 25.08 | 30 17 26.42 | ||||||||
Spectral type | DA | DA | DA | DA | DA | DA | DA | DA | DA | DA | |||||||
Effective temperature | [K] | 32669.0 (101) | 24725.0 | 32349.0 (417) | 34418.0 (580) | 32880.0 (90) | 32247.0 (956) | 33158.0 (65) | 32727.0 (43) | ||||||||
log(g) | [cgs] | 7.93 (0.02) | 7.31 | 8.00 (0.09) | 8.21 (0.1) | 7.88 (0.02) | 7.62 (0.03) | 7.90 (0.03) | 7.91 (0.02) | ||||||||
Mass | [M☉] | 0.61 (0.01) | 0.355 | 0.65 (0.05) | 0.78 (0.06) | 0.6 (0.01) | 0.477 (0.02) | 0.606 (0.009) | |||||||||
log(Luminosity) | [L☉] | -0.69 (0.01) | |||||||||||||||
Cooling age | [Gyr] | 0.0068 (0.0002) | 0.0166 | 0.0090 (0.001) | 0.0072 | ||||||||||||
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] | 4.18 (0.06) | 4.28 (0.1) | 4.18 | 4.18 (0.06) | ||||||||||||
Distance | [pc] | 239.25 (3) | 233.84 (6) | 156.00 | 239.25 | 239.25 (3) | |||||||||||
Composition | H | H | H | ||||||||||||||
Proper motion (right ascension) | [mas/yr] | 13.32990364 (0.07) | 13.38928138 (0.2) | 13.33 (0.07) | 15.5 | ||||||||||||
Proper motion (declination) | [mas/yr] | -11.55008839 (0.04) | -11.63632582 (0.08) | -11.55 (0.04) | -11.7 | ||||||||||||
Variability | |||||||||||||||||
Magnetic | |||||||||||||||||
Bd | [MG] | ||||||||||||||||
Infrared excess (disk) | |||||||||||||||||
Binarity | |||||||||||||||||
B magnitude | 15.20 | ||||||||||||||||
V magnitude | |||||||||||||||||
R magnitude | |||||||||||||||||
I magnitude | |||||||||||||||||
J magnitude | 16.73 (0.1) | ||||||||||||||||
H magnitude | |||||||||||||||||
K magnitude | |||||||||||||||||
u magnitude | 15.61 (0.005) | 15.65 | 15.61 (0.005) | 15.65 (0.01) | 15.64 | 15.62 (0.01) | |||||||||||
g magnitude | 15.85 (0.004) | 15.92 | 15.85 (0.004) | 15.92 (0.02) | 15.91 | 15.91 (0.02) | |||||||||||
r magnitude | 16.35 (0.004) | 16.39 | 16.35 (0.004) | 16.31 (0.02) | 16.30 (0.02) | ||||||||||||
i magnitude | 16.69 (0.005) | 16.72 | 16.69 (0.005) | 16.67 (0.02) | 16.68 (0.02) | ||||||||||||
z magnitude | 17.05 (0.01) | 17.05 | 17.05 (0.01) | 17.00 (0.02) | 17.00 (0.02) | ||||||||||||
G magnitude | 16.11 (0.003) | 16.14 | 16.11 | 16.11 (0.003) | |||||||||||||
BP magnitude | 15.98 (0.003) | 15.92 | |||||||||||||||
RP magnitude | 16.38 (0.004) | 16.38 | |||||||||||||||
Pan g magnitude | 15.95 (0.003) | ||||||||||||||||
Pan r magnitude | 16.35 (0.002) | ||||||||||||||||
Pan i magnitude | 16.70 (0.004) | ||||||||||||||||
Pan z magnitude | 16.98 (0.004) | ||||||||||||||||
Pan y magnitude | 17.16 (0.008) | ||||||||||||||||
E(B-V) | 0.016 |
* 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.