PG 1045+100

All names: PG1045+100, SDSS J104739.10+094424.1, SDSS J104739.10+094424.3, Gaia DR3 3869398301107963008, PG 1045+100, Gaia DR2 3869398301107963008, GALEX J104739.1+094424, SDSS J104739.10+094424.18, USNO-B1.0 0997-00211200, Gaia EDR3 3869398301107963008

Parameter Unit Gaia EDR3 Pan-STARRS DR1 SDSS DR10 Geier 2020 Gaia DR2 Stilism Kepler et al. 2015 Simbad
Right ascension 10 47 39.09 (0.08) 10 47 39.11 10 47 39.16 10 47 39.09 (0.1) 10 47 39.11 (0.08)
Declination 09 44 24.17 (0.06) 09 44 24.30 09 44 25.11 09 44 24.17 (0.1) 09 44 24.37 (0.06)
Spectral type He-sdO He-sdO sdOHe
Effective temperature [K] 46232.0 (2109) 47547.0 (45)
log(g) [cgs] 6.40 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] 0.05 (0.09) 0.06 (0.1) 0.06 (0.1) 0.05 (0.09)
Distance [pc] 19257.99 (31893) 15772.87 (25849) 15762.94 (25804) 19267.82 (31927)
Composition
Proper motion (right ascension) [mas/yr] -15.165503 (0.1) -14.974 (0.2) -14.97367502 (0.2) -15.166 (0.1)
Proper motion (declination) [mas/yr] -12.71311108 (0.1) -12.542 (0.2) -12.54244797 (0.2) -12.713 (0.1)
Variability
Magnetic
Bd [MG]
Infrared excess (disk)
Binarity
B magnitude 17.00
V magnitude
R magnitude 17.10
I magnitude
J magnitude 17.71 (0.03)
H magnitude 17.66 (0.07)
K magnitude 17.80 (0.1)
u magnitude 16.31 (0.006) 16.31 (0.006) 16.33 (0.01) 16.31 (0.006)
g magnitude 16.70 (0.004) 16.70 (0.004) 16.72 (0.02) 16.70 (0.004)
r magnitude 17.22 (0.005) 17.23 (0.005) 17.23 (0.02) 17.23 (0.005)
i magnitude 17.56 (0.007) 17.57 (0.007) 17.57 (0.02) 17.57 (0.007)
z magnitude 17.90 (0.02) 17.90 (0.02) 17.90 (0.03) 17.90 (0.02)
G magnitude 16.98 (0.008) 17.00 (0.004) 17.00 16.98 (0.003)
BP magnitude 16.84 (0.008) 16.76 (0.02) 16.76
RP magnitude 17.27 (0.01) 17.26 (0.01) 17.26
Pan g magnitude 16.80 (0.004) 16.80 (0.004)
Pan r magnitude 17.23 (0.003) 17.23 (0.003)
Pan i magnitude 17.61 (0.003) 17.61 (0.003)
Pan z magnitude 17.88 (0.005) 17.88 (0.005)
Pan y magnitude 18.09 (0.02) 18.09 (0.02)
E(B-V) 0.026

* 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.