WD 0804+446A

All names: PSO J080751.843+443030.449, Gaia DR2 929014482827319552, SDSS J080751.83+443030.4, WD 0804+446A, WD 0804+446.1, SDSS J080751.84+443030.5

Parameter Unit MWDD H Pan-STARRS DR1 Gaia DR2 SDSS DR12 Simbad Eisenstein et al. 2006 White Dwarf Catalog (McCook & Sion 1999) Kleinman et al. 2013 Kleinman et al. 2004
Right ascension 08 07 51.84 (0.7) 08 07 51.84 08 07 51.84 08 07 51.84 08 07 50.86 08 07 51.84 08 07 51.84
Declination 44 30 30.37 (0.6) 44 30 30.46 44 30 30.48 44 30 30.48 44 30 28.08 44 30 30.47 44 30 30.46
Spectral type DA DA DA DA1.4 DA
Effective temperature [K] 25217.0 36977.0 (1221) 36390.0 (1314) 37251.0 (1266)
log(g) [cgs] 8.89 7.87 (0.2) 7.76 (0.2) 7.90 (0.2)
Mass [M] 1.155 0.552 (0.09)
log(Luminosity) [L]
Cooling age [Gyr] 0.2059
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] 2.53 (1)
Distance [pc] 395.59 (153)
Composition H
Proper motion (right ascension) [mas/yr] 2.710633389 (1) -3.0 -3.0 -4.0
Proper motion (declination) [mas/yr] -4.496380592 (1) 1.0 -2.7 0.0
Variability
Magnetic
Bd [MG]
Infrared excess (disk)
Binarity
B magnitude
V magnitude
R magnitude
I magnitude
J magnitude
H magnitude
K magnitude
u magnitude 19.50 (0.03) 19.50 19.52 (0.03) 19.50 19.52 (0.03) 19.50 (0.03)
g magnitude 19.80 (0.01) 19.79 19.82 (0.02) 19.82 19.82 (0.02) 19.82 (0.02)
r magnitude 20.26 (0.03) 20.26 20.29 (0.03) 20.29 20.28 (0.03) 20.29 (0.03)
i magnitude 20.58 (0.04) 20.58 20.61 (0.04) 20.60 20.61 (0.04) 20.60 (0.04)
z magnitude 20.65 (0.2) 20.68 20.68 (0.2) 20.69 20.67 (0.2) 20.69 (0.2)
G magnitude 20.15
BP magnitude 20.11
RP magnitude 20.25
Pan g magnitude 19.84 (0.02)
Pan r magnitude 20.33 (0.03)
Pan i magnitude 20.63 (0.03)
Pan z magnitude 20.81 (0.2)
Pan y magnitude

* Constant surface field

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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.