All names: 23082+2414, WD 2305+239, Gaia DR2 2842462137347560320, SDSS J230812.82+241425.0, Gaia EDR3 2842462137347560320, PSO J347.0539+24.2401, J2308+2414, NLTT 55920, WDJ230812.71+241425.53, LP 401-50, TIC 436834270, PM J23082+2414, Gaia DR3 2842462137347560320, USNO-B1.0 1142-00554204, LSPM J2308+2414, 2MASS J23081266+2414255
Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | O'Brien et al. 2024 | Caron et al. 2023 | McCleery et al. 2020 | Blouin et al. 2019 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Limoges et al. 2015 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 | White Dwarf Catalog (McCook & Sion 1999) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Right ascension | 23 08 12.98 (0.09) | 23 08 12.97 (0.1) | 23 08 12.97 (0.1) | 23 08 12.98 | 23 08 12.71 (0.09) | 23 08 12.97 | 23 08 14.93 | |||||||||
Declination | 24 14 24.34 (0.08) | 24 14 24.37 (0.09) | 24 14 24.37 (0.09) | 24 14 24.34 | 24 14 25.53 (0.08) | 24 14 24.37 | 24 14 15.36 | |||||||||
Spectral type | DC | DC | DC | DC | DC | DC | DC | DA: | DC | DC | ||||||
Effective temperature | [K] | 4898.0 (84) | 4798.0 (19) | 4786.4 (47) | 4825.0 (25) | 4849.0 | 4528.0 | 4760.0 (105) | 4884.0 (49) | |||||||
log(g) | [cgs] | 7.88 (0.07) | 7.85 (0.01) | 7.84 (0.04) | 7.86 (0.02) | 7.88 | 7.65 | 8.00 (0) | 7.89 (0.03) | |||||||
Mass | [M☉] | 0.511 (0.04) | 0.493 (0.01) | 0.498 (0.01) | 0.508 | 0.378 | 0.58 (0.1) | 0.515 (0.02) | ||||||||
log(Luminosity) | [L☉] | -4.14 | ||||||||||||||
Cooling age | [Gyr] | 5.2100 | 4.9410 (0.3) | 5.0160 | 3.7230 | |||||||||||
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] | 25.00 (0.1) | 25.00 (0.1) | 25.21 (0.1) | 25.21 (0.2) | 25.21 (0.2) | 25.21 (0.2) | 25.00 | 25.00 (0.1) | 25.21 (0.2) | ||||||
Distance | [pc] | 40.00 (0.2) | 40.00 (0.2) | 39.67 (0.2) | 39.67 (0.2) | 39.67 (0.2) | 39.67 (0.2) | 35.10 (6) | 40.00 | 40.00 (0.2) | 39.67 (0.2) | |||||
Composition | H | H | H | |||||||||||||
Proper motion (right ascension) | [mas/yr] | 233.2140107 (0.1) | 233.4946186 (0.2) | 233.214 (0.1) | 233.4946186 | |||||||||||
Proper motion (declination) | [mas/yr] | -74.67599761 (0.1) | -74.89671686 (0.2) | -74.676 (0.1) | -74.89671686 | |||||||||||
Variability | ||||||||||||||||
Magnetic | ||||||||||||||||
Bd | [MG] | |||||||||||||||
Infrared excess (disk) | ||||||||||||||||
Binarity | yes | |||||||||||||||
B magnitude | 18.60 | |||||||||||||||
V magnitude | ||||||||||||||||
R magnitude | 17.40 | |||||||||||||||
I magnitude | ||||||||||||||||
J magnitude | 16.50 (0.02) | 16.55 (0.1) | 16.55 (0.1) | |||||||||||||
H magnitude | ||||||||||||||||
K magnitude | ||||||||||||||||
u magnitude | 20.46 (0.07) | 20.47 (0.07) | 20.47 (0.07) | |||||||||||||
g magnitude | 18.49 (0.006) | 18.56 (0.008) | ||||||||||||||
r magnitude | 17.80 (0.003) | 17.82 (0.006) | ||||||||||||||
i magnitude | 17.54 (0.006) | 17.52 (0.007) | ||||||||||||||
z magnitude | 17.44 (0.01) | 17.39 (0.01) | ||||||||||||||
G magnitude | 17.84 (0.02) | 17.87 | 17.87 | 17.84 | 17.84 (0.003) | 17.87 | ||||||||||
BP magnitude | 18.36 (0.02) | 18.39 | 18.39 | |||||||||||||
RP magnitude | 17.19 (0.01) | 17.20 | 17.20 | |||||||||||||
Pan g magnitude | 18.49 (0.008) | 18.49 (0.006) | 18.49 (0.006) | |||||||||||||
Pan r magnitude | 17.80 (0.004) | 17.80 (0.003) | 17.80 (0.003) | |||||||||||||
Pan i magnitude | 17.54 (0.005) | 17.54 (0.006) | 17.54 (0.006) | |||||||||||||
Pan z magnitude | 17.44 (0.008) | 17.44 (0.01) | 17.44 (0.01) | |||||||||||||
Pan y magnitude | 17.39 (0.007) | 17.39 (0.007) | 17.39 (0.007) | |||||||||||||
E(B-V) | 0.002 |
* Constant surface field
Spectra without link are available upon request
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.