SDSS J112926.23+493931.8

All names: NAME SDSS J112924.74+493931.9, SDSS J112926.23+493931.9, WD 1126+499, SDSS J112926.23+493931.8, PSO J112926.269+493931.498, Gaia DR2 790041302613954944

Parameter Unit MWDD H Pan-STARRS DR1 Gaia DR2 Kulebi et al. 2009 SDSS DR12 Simbad Eisenstein et al. 2006 Kleinman et al. 2013
Right ascension 11 29 26.28 (0.09) 11 29 26.23 11 29 26.23 11 29 26.23 11 29 26.23 11 29 26.23
Declination 49 39 31.27 (0.1) 49 39 31.79 49 39 31.82 49 39 31.83 49 39 31.85 49 39 31.86
Spectral type DAH DAH DAH DAH DAH
Effective temperature [K] 9774.0 19664.0 (207) 20160.0 (210)
log(g) [cgs] 8.05 8.00 (0) 9.00 (0.001) 9.33 (0.04)
Mass [M] 0.63
log(Luminosity) [L]
Cooling age [Gyr] 0.6876
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] 7.38 (0.1)
Distance [pc] 135.52 (3)
Composition H H
Proper motion (right ascension) [mas/yr] 35.0253623868 (0.1) 32.0 36.0
Proper motion (declination) [mas/yr] -40.3065951568 (0.2) -47.0 -50.2
Variability
Magnetic yes yes
Bd [MG] 5.31 (0.6)
Infrared excess (disk)
Binarity
B magnitude
V magnitude
R magnitude
I magnitude
J magnitude
H magnitude
K magnitude
u magnitude 18.45 (0.02) 18.45 18.42 (0.05) 18.45 (0.05)
g magnitude 18.00 (0.006) 18.02 18.00 (0.02) 18.02 (0.02)
r magnitude 18.07 (0.007) 18.08 18.08 (0.01) 18.08 (0.01)
i magnitude 18.18 (0.008) 18.15 18.15 (0.02) 18.15 (0.02)
z magnitude 18.33 (0.02) 18.34 18.34 (0.03) 18.34 (0.03)
G magnitude 18.01
BP magnitude 18.04
RP magnitude 17.90
Pan g magnitude 17.99 (0.01)
Pan r magnitude 18.06 (0.008)
Pan i magnitude 18.19 (0.004)
Pan z magnitude 18.35 (0.007)
Pan y magnitude 18.46 (0.01)

* Constant surface field

Special notes:

Spectra

Controls

Normalize at:

Range:

x: to
y: to

Spectra available:

Spectra without link are available upon request

Absorption lines

Photometric filters

BVRI
ugriz

Photometric fit





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.