SDSS J102241.20+203839.6

All names: Gaia DR3 625619814102557568, SDSSJ102241.20+203839.6, Gaia EDR3 625619814102557568, SDSS J102241.21+203839.6, SDSS J102241.21+203839.62, Gaia DR2 625619814102557568, SDSS J102241.20+203839.6

Parameter Unit Gaia EDR3 Pan-STARRS DR1 SDSS DR10 Geier 2020 Gaia DR2 Stilism Kepler et al. 2015 Simbad
Right ascension 10 22 41.21 (0.1) 10 22 41.20 10 22 41.20 10 22 41.21 (0.2) 10 22 41.21 (0.1)
Declination 20 38 39.63 (0.1) 20 38 39.62 20 38 39.60 20 38 39.63 (0.2) 20 38 39.66 (0.1)
Spectral type He-sdO He-sdO: sdOHe
Effective temperature [K] 48462.0 (47)
log(g) [cgs] 7.00 (0.05)
Mass [M]
log(Luminosity) [L]
Cooling age [Gyr]
log(H/He)
log(C/He)
log(Ca/He)
log(Ca/H)
Parallax [mas] 0.16 (0.2) 0.31 (0.2) 0.31 (0.2) 0.16 (0.2)
Distance [pc] 6160.60 (6243) 3258.39 (2291) 3258.77 (2291) 6161.43 (6245)
Composition
Proper motion (right ascension) [mas/yr] -1.860515834 (0.2) -1.464 (0.4) -1.463570476 (0.4) -1.861 (0.2)
Proper motion (declination) [mas/yr] -1.940652952 (0.1) -1.73 (0.3) -1.730023226 (0.3) -1.941 (0.1)
Variability
Magnetic
Bd [MG]
Infrared excess (disk)
Binarity
B magnitude
V magnitude
R magnitude
I magnitude
J magnitude
H magnitude
K magnitude
u magnitude 17.53 (0.01) 17.53 (0.01) 17.54 (0.02) 17.53 (0.01)
g magnitude 17.97 (0.006) 17.97 (0.006) 18.00 (0.02) 17.97 (0.006)
r magnitude 18.50 (0.009) 18.50 (0.009) 18.52 (0.02) 18.50 (0.009)
i magnitude 18.84 (0.01) 18.84 (0.01) 18.85 (0.04) 18.84 (0.01)
z magnitude 19.23 (0.04) 19.23 (0.04) 19.25 (0.05) 19.23 (0.04)
G magnitude 18.25 (0.01) 18.31 (0.005) 18.31 18.25 (0.003)
BP magnitude 18.11 (0.01) 18.13 (0.03) 18.13
RP magnitude 18.58 (0.03) 18.51 (0.06) 18.51
Pan g magnitude 18.07 (0.008) 18.07 (0.008)
Pan r magnitude 18.51 (0.008) 18.51 (0.008)
Pan i magnitude 18.87 (0.01) 18.87 (0.01)
Pan z magnitude 19.14 (0.03) 19.14 (0.03)
Pan y magnitude 19.31 (0.03) 19.31 (0.03)
E(B-V) 0.020

* Constant surface field

Special notes:

Spectra

Controls

Normalize at:
Normalize by mean flux

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 (Université de Montréal) and Dr. Simon Blouin (University of Victoria). Please send database updates, corrections, suggestions or bug reports to patrick.dufour@umontreal.ca.