All names: PLX 2716, AC2000 4195112, ALS 2481, BPM 7108, CSI-64-11430, CSI-64-11431, Ci 20 658, EGGR 82, GEN# +9.86145141, GJ 440, GSC 08981-04418, GSC 08981-04378, GSC 08981-04417, HIC 57367, HIP 57367, L 145-41, L 145-141, LAWD 37, LFT 844, LHS 43, LP 145-141, LPM 396, LS 2481, LTT 4364, NLTT 28447, PM 11429-6434, UBV M 42331, UBV 10596, WD 1141-64, WD 1142-64, WD 1142-645, WG 20, Zkh 167, [L68] 74, uvby98 986145141, 2MASS J11454297-6450297, PLX 2716.00, TYC 8981-4417-1
Parameter | Unit | Holberg et al. 2016 | Sion et al. 2014 | Koester et al. 1982a | Simbad |
---|---|---|---|---|---|
Right ascension | 11 45 49.92 | 11 45 42.92 | |||
Declination | -64 50 27.60 | -64 50 29.46 | |||
Spectral type | DQ | DQ6.4 | DQ | DQ | |
Effective temperature | [K] | 7972.0 (219) | 7966.0 | 7800.0 (200) | |
log(g) | [cgs] | 7.88 (0.02) | |||
Mass | [M☉] | 0.61 (0.01) | 0.46 (0.06) | ||
log(Luminosity) | [L☉] | ||||
Cooling age | [Gyr] | 1.2900 | |||
log(H/He) | |||||
log(C/He) | -5.4 | ||||
log(Ca/He) | |||||
log(Ca/H) | |||||
log(N/He) | |||||
log(O/He) | |||||
log(Na/He) | |||||
log(Mg/He) | |||||
log(Al/He) | |||||
log(Si/He) | |||||
log(P/He) | |||||
log(S/He) | |||||
log(Cl/He) | |||||
log(Sc/He) | |||||
log(Ti/He) | |||||
log(V/He) | |||||
log(Cr/He) | |||||
log(Mn/He) | |||||
log(Fe/He) | |||||
log(Co/He) | |||||
log(Ni/He) | |||||
log(Cu/He) | |||||
log(Zn/He) | |||||
log(Ga/He) | |||||
log(Ge/He) | |||||
log(Sr/He) | |||||
Parallax | [mas] | 216.12 (1) | 215.80 | ||
Distance | [pc] | 4.63 (0.02) | 4.62 | 4.63 | |
Composition | He | ||||
Proper motion (right ascension) | [mas/yr] | 2668.5 | |||
Proper motion (declination) | [mas/yr] | -352.7 | |||
Variability | |||||
Magnetic | |||||
Bd | [MG] | ||||
Infrared excess (disk) | |||||
Binarity | |||||
B magnitude | 11.72 | ||||
V magnitude | 11.50 | 11.51 | |||
R magnitude | 11.34 | ||||
I magnitude | 11.16 | ||||
J magnitude | 11.19 | ||||
H magnitude | 11.13 | ||||
K magnitude | 11.10 | ||||
u magnitude | |||||
g magnitude | |||||
r magnitude | |||||
i magnitude | |||||
z magnitude |
* 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.