All names: LAMOST J084104.01+392307.3, SDSS J084104.02+392307.3, KUV 08378+3934, PSO J084104.016+392307.511, Gaia DR2 910801931705082752, SDSS J084104.02+392307.33
Parameter | Unit | MWDD H | Pan-STARRS DR1 | Gaia DR2 | Kepler et al. 2015 | SDSS DR10 | Simbad |
---|---|---|---|---|---|---|---|
Right ascension | 08 41 04.01 (0.07) | 08 41 04.02 | 08 41 04.02 | ||||
Declination | 39 23 07.43 (0.05) | 39 23 07.45 | 39 23 07.45 | ||||
Spectral type | DA | DA | DA2.3 | ||||
Effective temperature | [K] | 19894.0 | 21561.0 (72) | ||||
log(g) | [cgs] | 7.91 | 8.11 (0.01) | ||||
Mass | [M☉] | 0.574 | 0.6829999999999999 (0.005) | ||||
log(Luminosity) | [L☉] | ||||||
Cooling age | [Gyr] | 0.0558 | |||||
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] | 6.55 (0.08) | |||||
Distance | [pc] | 152.63 (2) | |||||
Composition | H | ||||||
Proper motion (right ascension) | [mas/yr] | -9.2224013267 (0.1) | -10.0 | ||||
Proper motion (declination) | [mas/yr] | -4.774165356 (0.1) | -8.0 | ||||
Variability | |||||||
Magnetic | |||||||
Bd | [MG] | ||||||
Infrared excess (disk) | |||||||
Binarity | |||||||
B magnitude | |||||||
V magnitude | 16.54 | ||||||
R magnitude | |||||||
I magnitude | |||||||
J magnitude | |||||||
H magnitude | |||||||
K magnitude | |||||||
u magnitude | 16.37 (0.02) | 16.40 (0.006) | 16.40 | ||||
g magnitude | 16.37 (0.01) | 16.36 (0.004) | 16.36 | ||||
r magnitude | 16.75 (0.01) | 16.74 (0.004) | 16.74 | ||||
i magnitude | 17.06 (0.01) | 17.05 (0.005) | 17.05 | ||||
z magnitude | 17.37 (0.02) | 17.36 (0.01) | 17.36 | ||||
G magnitude | 16.61 | ||||||
BP magnitude | 16.47 | ||||||
RP magnitude | 16.78 | ||||||
Pan g magnitude | 16.42 (0.005) | ||||||
Pan r magnitude | 16.76 (0.005) | ||||||
Pan i magnitude | 17.08 (0.003) | ||||||
Pan z magnitude | 17.35 (0.003) | ||||||
Pan y magnitude | 17.53 (0.02) |
* 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.