All names: G 149-7, WDS J12472+1442BC, G 61-17, uvby98 600118245, ** EGG 7, 2MASS J12471477+1442307, WD 1244+15, ** GIC 109B, WDJ124714.71+144230.88, USNO-B1.0 1047-00215871, PLX 2941.02, PG 1244+149, GCRV 63553, G61-17, J1247+1442, Gaia DR2 3930922058356114560, LTT 18245, NLTT 31890, SDSS J124714.61+144231.5, WD 1244+149, WD 1244+14, TIC 92043865, LSPM J1247+1442E, CSI+14-12448, USNO 733, WD 1244+145, UBV 11487, Gaia EDR3 3930922058356114560, Gaia DR3 3930922058356114560, EGGR 92, GEN# +9.80061017
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | Kilic et al. 2020 | MWDD H | Gaia DR2 | Stilism | Gianninas et al. 2011 | Liebert et al. 2005 | Bergeron et al. 2001 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 12 47 14.32 (0.04) | 12 47 14.33 (0.05) | 12 47 14.32 | 12 47 14.71 (0.04) | 12 47 14.33 | 12 47 15.24 | |||||||||
Declination | 14 42 33.25 (0.02) | 14 42 33.18 (0.04) | 14 42 33.25 | 14 42 30.88 (0.02) | 14 42 33.18 | 14 42 25.92 | |||||||||
Spectral type | DA | DA | DA | DA | DA | DA | DA4.6 | DA5 | |||||||
Effective temperature | [K] | 10482.0 (29) | 10482.0 (29) | 10482.0 | 10870.0 (161) | 10680.0 (156) | 10280.0 (310) | 10488.0 (65) | |||||||
log(g) | [cgs] | 7.96 (0.005) | 7.96 (0.005) | 7.96 | 8.15 (0.05) | 8.06 (0.05) | 7.88 (0.4) | 7.96 (0.01) | |||||||
Mass | [M☉] | 0.576 (0.004) | 0.576 (0.004) | 0.577 | 0.69 (0.03) | 0.64 (0.03) | 0.53 (0.2) | 0.578 (0.008) | |||||||
log(Luminosity) | [L☉] | -2.75 | -2.71 (0.2) | ||||||||||||
Cooling age | [Gyr] | 0.5042 | 0.6310 | 0.4800 (0.2) | |||||||||||
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] | 16.39 (0.05) | 16.39 (0.05) | 15.70 (4) | 16.39 | 16.39 (0.05) | 16.39 (0.05) | 14.40 (42) | |||||||
Distance | [pc] | 60.99 (0.2) | 61.00 (0.2) | 55.00 | 59.00 | 63.69 (17) | 60.99 | 60.99 (0.2) | 61.00 (0.2) | 69.44 (203) | |||||
Composition | H | H | H | H | |||||||||||
Proper motion (right ascension) | [mas/yr] | -354.3813646 (0.05) | -354.5812355 (0.1) | -354.381 (0.05) | -354.5812355 | ||||||||||
Proper motion (declination) | [mas/yr] | 148.668455 (0.05) | 148.5636559 (0.07) | 148.668 (0.05) | 148.5636559 | ||||||||||
Variability | NOV | ||||||||||||||
Magnetic | |||||||||||||||
Bd | [MG] | ||||||||||||||
Infrared excess (disk) | |||||||||||||||
Binarity | yes | ||||||||||||||
B magnitude | 16.06 | 16.08 | |||||||||||||
V magnitude | 15.90 | 15.89 | |||||||||||||
R magnitude | 15.86 | 15.90 | |||||||||||||
I magnitude | 15.83 | ||||||||||||||
J magnitude | 15.84 | 15.88 (0.008) | |||||||||||||
H magnitude | 15.86 | 15.86 (0.01) | |||||||||||||
K magnitude | 15.84 | 15.90 (0.03) | |||||||||||||
u magnitude | 16.32 (0.006) | 16.32 (0.006) | 16.24 | ||||||||||||
g magnitude | 15.87 (0.004) | 15.87 (0.004) | 15.85 | ||||||||||||
r magnitude | 15.96 (0.005) | 15.96 (0.005) | 15.94 | ||||||||||||
i magnitude | 16.13 (0.005) | 16.13 (0.005) | 16.14 | ||||||||||||
z magnitude | 16.32 (0.008) | 16.32 (0.008) | 16.36 | ||||||||||||
G magnitude | 15.89 (0.002) | 15.91 | 15.89 | 15.89 (0.003) | 15.91 | ||||||||||
BP magnitude | 15.93 (0.002) | 15.93 | 15.93 | ||||||||||||
RP magnitude | 15.83 (0.004) | 15.84 | 15.84 | ||||||||||||
Pan g magnitude | 15.86 (0.002) | ||||||||||||||
Pan r magnitude | 15.98 (0.002) | ||||||||||||||
Pan i magnitude | 16.14 (0.0004) | ||||||||||||||
Pan z magnitude | 16.33 (0.01) | ||||||||||||||
Pan y magnitude | 16.45 (0.02) | ||||||||||||||
E(B-V) | 0.002 |
* 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.