All names: [MMN2004c] WD J1450+5543, TIC 310003064, GALEX J145040.4+554321, [HHD2009] SDSS J1450+5543, SDSS J145040.49+554321.4, WIRED J145040.50+554321.4, SDSS J145040.50+554321.3, LAMOST J145040.45+554321.0, SDSS J145040.50+554321.4, Gaia EDR3 1607402196407329536, 2MASS J14504049+5543217, Gaia DR3 1607402196407329536, Gaia DR2 1607402196407329536, [SGR2010] J1450+5543, WD 1449+559
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR12 | MWDD H | Gaia DR2 | Stilism | sdss-wdms.org (29/04/2016) | Guo et al. 2015 | Tremblay et al. 2011 | Mukadam et al. 2004 | 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 | 14 50 40.42 (0.06) | 14 50 40.49 | 14 50 40.42 (0.07) | 14 50 40.50 | 14 50 40.42 | 14 50 40.50 (0.06) | 14 50 40.50 | 14 50 40.32 | 14 50 40.50 | ||||||||
Declination | 55 43 21.91 (0.06) | 55 43 21.41 | 55 43 21.89 (0.07) | 55 43 21.40 | 55 43 21.91 | 55 43 21.32 (0.06) | 55 43 21.32 | 55 43 17.04 | 55 43 21.42 | ||||||||
Spectral type | DA+M | DA+M | DA | DA | DA | DA+dM | DA+M: | DA3.4 | DA+M | DA+MS | |||||||
Effective temperature | [K] | 10567.0 | 15422.0 (203) | 16480.0 (190) | 15010.0 (120) | 9082.0 (81) | 15013.0 (121) | 15413.0 (123) | |||||||||
log(g) | [cgs] | 7.01 | 7.60 (0.04) | 7.77 (0.04) | 7.48 (0.03) | 6.52 (0.04) | 7.48 (0.03) | 7.56 (0.03) | |||||||||
Mass | [M☉] | 0.224 | 0.41 (0.02) | 0.49 (0.02) | 0.122 (0.009) | ||||||||||||
log(Luminosity) | [L☉] | ||||||||||||||||
Cooling age | [Gyr] | 0.1963 | 0.1000 | ||||||||||||||
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] | 4.40 (0.06) | 4.43 (0.08) | 4.40 | 4.39 (0.06) | ||||||||||||
Distance | [pc] | 227.53 (3) | 225.83 (4) | 256.00 (35) | 227.53 | 227.53 (3) | |||||||||||
Composition | H | H | |||||||||||||||
Proper motion (right ascension) | [mas/yr] | -43.63710696 (0.07) | -43.69305937 (0.1) | -43.637 (0.07) | -39.5 | ||||||||||||
Proper motion (declination) | [mas/yr] | 36.82246147 (0.08) | 36.65382651 (0.1) | 36.822 (0.08) | 33.4 | ||||||||||||
Variability | NOV | ||||||||||||||||
Magnetic | |||||||||||||||||
Bd | [MG] | ||||||||||||||||
Infrared excess (disk) | |||||||||||||||||
Binarity | WDMS | WDMS | WDMS | WDMS | |||||||||||||
B magnitude | |||||||||||||||||
V magnitude | |||||||||||||||||
R magnitude | |||||||||||||||||
I magnitude | |||||||||||||||||
J magnitude | 16.24 (0.1) | ||||||||||||||||
H magnitude | 15.96 (0.2) | ||||||||||||||||
K magnitude | 15.31 (0.1) | ||||||||||||||||
u magnitude | 17.53 (0.01) | 17.55 | 17.53 (0.01) | 17.55 (0.02) | 17.52 | 17.54 (0.02) | |||||||||||
g magnitude | 17.20 (0.004) | 17.20 | 17.21 | 17.20 (0.004) | 17.20 (0.02) | 17.21 | 17.19 (0.02) | ||||||||||
r magnitude | 17.51 (0.005) | 17.51 | 17.51 (0.005) | 17.51 (0.02) | 17.50 (0.02) | ||||||||||||
i magnitude | 17.58 (0.006) | 17.58 | 17.58 (0.006) | 17.58 (0.02) | 17.58 (0.02) | ||||||||||||
z magnitude | 17.39 (0.01) | 17.38 | 17.39 (0.01) | 17.38 (0.02) | 17.38 (0.02) | ||||||||||||
G magnitude | 17.32 (0.007) | 17.35 | 17.32 | 17.32 (0.003) | |||||||||||||
BP magnitude | 17.36 (0.007) | 17.33 | |||||||||||||||
RP magnitude | 17.21 (0.008) | 17.19 | |||||||||||||||
Pan g magnitude | 17.26 (0.005) | ||||||||||||||||
Pan r magnitude | 17.52 (0.006) | ||||||||||||||||
Pan i magnitude | 17.60 (0.006) | ||||||||||||||||
Pan z magnitude | 17.49 (0.007) | ||||||||||||||||
Pan y magnitude | 17.33 (0.01) | ||||||||||||||||
E(B-V) | 0.018 |
* 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.