All names: Feige 44, USNO-B1.0 1052-00205424, PG 1129+155, WD 1129+155, 11324+1517, 1SWASP J113227.35+151731.0, Gaia DR3 3966519331420622080, PM J11324+1517, GALEX J113227.3+151729, SDSS J113227.37+151730.6, TIC 165427922, LAMOST J113227.34+151731.0, WD 1129+156, LAMOST J113227.35+151730.8, Gaia DR2 3966519331420622080, [TFW97] J113227.37+151731.20, 2MASS J11322734+1517310, CHSS 1944, LAMOST J113227.41+151729.3, PG 1129+156, WDJ113227.36+151730.81, Gaia EDR3 3966519331420622080, GSC 01438-00055
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | MWDD H | Gaia DR2 | Stilism | Guo et al. 2015 | Limoges et al. 2015 | Koester et al. 2014 | Gianninas et al. 2011 | Koester et al. 2009 | Liebert et al. 2005 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 11 32 27.41 (0.1) | 11 32 27.41 (0.1) | 11 32 27.41 | 11 32 27.36 (0.1) | 11 32 27.41 | 11 32 27.07 | |||||||||||
Declination | 15 17 30.08 (0.1) | 15 17 30.10 (0.1) | 15 17 30.08 | 15 17 30.82 (0.1) | 15 17 30.10 | 15 17 37.68 | |||||||||||
Spectral type | DA | DA | DA | DA | DA | DA | DA2.8 | DA4 | |||||||||
Effective temperature | [K] | 17417.0 (164) | 16141.0 | 18239.0 (67) | 17990.0 (277) | 18915.0 (257) | 17990.0 (279) | 17739.0 (16) | 16890.0 (261) | 16368.0 (159) | |||||||
log(g) | [cgs] | 7.74 (0.01) | 7.71 | 8.27 (0.01) | 8.24 (0.05) | 8.19 (0.09) | 8.24 (0.05) | 8.03 (0.003) | 8.19 (0.05) | 7.67 (0.01) | |||||||
Mass | [M☉] | 0.483 (0.007) | 0.467 | 0.78 (0.01) | 0.77 (0.03) | 0.725 (0.05) | 0.76 (0.03) | 0.73 (0.03) | 0.446 (0.007) | ||||||||
log(Luminosity) | [L☉] | -1.95 | -2.02 | ||||||||||||||
Cooling age | [Gyr] | 0.0954 | 0.2239 | ||||||||||||||
log(H/He) | |||||||||||||||||
log(C/He) | |||||||||||||||||
log(Ca/He) | |||||||||||||||||
log(Ca/H) | |||||||||||||||||
log(C/H) | <-8.10 | ||||||||||||||||
log(N/H) | |||||||||||||||||
log(O/H) | |||||||||||||||||
log(Na/H) | |||||||||||||||||
log(Mg/H) | |||||||||||||||||
log(Al/H) | |||||||||||||||||
log(Si/H) | -8.3 (0.2) | ||||||||||||||||
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] | 20.47 (0.1) | 21.33 (0.1) | 20.47 | 20.47 (0.1) | 21.33 (0.1) | |||||||||||
Distance | [pc] | 48.86 (0.3) | 46.88 (0.3) | 35.80 (2) | 35.00 | 36.00 | 48.86 | 48.86 (0.3) | 46.88 (0.3) | ||||||||
Composition | H | H | H | H | |||||||||||||
Proper motion (right ascension) | [mas/yr] | 47.12583435 (0.2) | 47.80015547 (0.3) | 47.126 (0.2) | 47.80015547 | ||||||||||||
Proper motion (declination) | [mas/yr] | -46.25324459 (0.1) | -45.91645639 (0.2) | -46.253 (0.1) | -45.91645639 | ||||||||||||
Variability | |||||||||||||||||
Magnetic | |||||||||||||||||
Bd | [MG] | ||||||||||||||||
Infrared excess (disk) | |||||||||||||||||
Binarity | |||||||||||||||||
B magnitude | 14.03 | ||||||||||||||||
V magnitude | 14.09 (0.05) | 14.04 | 14.09 | 14.26 | |||||||||||||
R magnitude | 14.50 | ||||||||||||||||
I magnitude | |||||||||||||||||
J magnitude | 14.44 (0.03) | ||||||||||||||||
H magnitude | 14.49 (0.05) | ||||||||||||||||
K magnitude | 14.56 (0.09) | ||||||||||||||||
u magnitude | 14.90 (0.008) | 14.90 (0.008) | |||||||||||||||
g magnitude | 14.62 (0.005) | 14.62 (0.005) | |||||||||||||||
r magnitude | 14.33 (0.003) | 14.33 (0.003) | |||||||||||||||
i magnitude | 15.25 (0.009) | 15.25 (0.009) | |||||||||||||||
z magnitude | 15.26 (0.008) | 15.26 (0.008) | |||||||||||||||
G magnitude | 14.12 (0.001) | 14.14 | 14.12 | 14.12 (0.003) | 14.14 | ||||||||||||
BP magnitude | 14.07 (0.001) | 14.05 | 14.05 | ||||||||||||||
RP magnitude | 14.25 (0.002) | 14.26 | 14.26 | ||||||||||||||
Pan g magnitude | 13.98 (0.004) | ||||||||||||||||
Pan r magnitude | 14.28 (0.001) | ||||||||||||||||
Pan i magnitude | 14.59 (0.002) | ||||||||||||||||
Pan z magnitude | 14.82 (0.004) | ||||||||||||||||
Pan y magnitude | 14.97 (0.009) | ||||||||||||||||
E(B-V) | 0.001 |
* 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.