All names: NLTT 7948, 2MASS J02255196+4228042, Gaia DR2 339492017717622016, Gaia DR2 341372212664612608, USNO-B1.0 1324-00053079, KUV 02245+3145, LP 197-5, WDJ022551.96+422803.52, 02258+4228W, PSO J022552.411+422800.915, PSO J022552.460+422800.625, WD 0222+422.2, WD 0222+422B, WD 0222+422, WD 0224+317, USNO-B1.0 1219-00031966, LSPM J0225+4228W
Parameter | Unit | Blouin et al. 2019 | MWDD H | Pan-STARRS DR1 | Gaia DR2 | Limoges et al. 2015 | Gianninas et al. 2011 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 02 25 52.52 (0.1) | 02 25 51.96 | 02 25 52.52 | 02 25 51.62 | ||||||
Declination | 42 28 00.32 (0.1) | 42 28 04.30 | 42 28 00.32 | 42 28 30.00 | ||||||
Spectral type | DA | DA | DA | DA | DA8.0 | DA | ||||
Effective temperature | [K] | 6190.0 (65) | 6213.0 | 5410.0 (177) | 6320.0 (280) | |||||
log(g) | [cgs] | 7.94 (0.03) | 7.94 | 8.00 (0) | 8.17 (0.6) | |||||
Mass | [M☉] | 0.5529999999999999 (0.02) | 0.555 | 0.58 (0.1) | 0.69 (0.3) | |||||
log(Luminosity) | [L☉] | -3.91 | ||||||||
Cooling age | [Gyr] | 1.8740 (0.1) | 1.8620 | |||||||
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] | 19.82 (0.2) | 19.82 (0.2) | 19.82 (0.2) | ||||||
Distance | [pc] | 50.45 (0.4) | 50.45 (0.4) | 38.10 (2) | 41.00 | 50.45 (0.4) | ||||
Composition | H | H | H | |||||||
Proper motion (right ascension) | [mas/yr] | 397.4046392 (0.2) | 411.0 | 397.4046392 | ||||||
Proper motion (declination) | [mas/yr] | -206.7686543 (0.2) | -208.0 | -206.7686543 | ||||||
Variability | ||||||||||
Magnetic | ||||||||||
Bd | [MG] | |||||||||
Infrared excess (disk) | ||||||||||
Binarity | yes | |||||||||
B magnitude | 16.00 | |||||||||
V magnitude | 17.33 | |||||||||
R magnitude | 16.70 | |||||||||
I magnitude | 16.80 | |||||||||
J magnitude | 16.50 (0.1) | 16.50 | ||||||||
H magnitude | 16.26 (0.2) | 16.26 | ||||||||
K magnitude | 16.17 (0.2) | 16.17 | ||||||||
u magnitude | ||||||||||
g magnitude | ||||||||||
r magnitude | ||||||||||
i magnitude | ||||||||||
z magnitude | ||||||||||
G magnitude | 17.33 | 17.33 | ||||||||
BP magnitude | 17.58 | 17.58 | ||||||||
RP magnitude | 16.89 | 16.89 | ||||||||
Pan g magnitude | 17.61 (0.01) | 17.60 (0.002) | ||||||||
Pan r magnitude | 17.32 (0.004) | 17.33 (0.002) | ||||||||
Pan i magnitude | 17.21 (0.004) | 17.21 (0.006) | ||||||||
Pan z magnitude | 17.23 (0.003) | 17.22 (0.005) | ||||||||
Pan y magnitude | 17.22 (0.02) | 17.24 (0.007) |
* Constant surface field
Spectra without link are available upon request
The Montreal White Dwarf Database is produced and maintained by Prof. Patrick Dufour at Université de Montréal. Please send database updates, corrections, suggestions or bug reports to dufourpa@astro.umontreal.ca.