CONFIRMED
LMC
|
LMC S63 | IRAS - | GSC2.4.2 S1HC367984 | AAVSO 000-BJP-583 |
SIMBAD LHA 120-S 63 | Pan-STARRS - | SAO - | VSX 237639 |
GAIA DR3 4659219795902825600 | SkyMapper 054843.44-673610.4 | WRAY - | GCVS - |
2MASS J05484342-6736102 | HIP - | Hen - | BD - |
WISE J054843.42-673610.2 | TYC - | ESO - | HD - |
Bidelman (1954) | - | Allen (1984) | LMC S63 (Conf.) | Belzcyński et al. (2001) | LMC S63 (Conf.) |
Gaposchkin (1957) | - | Kenyon (1986) | LMC S63 (Conf.) | Akras et al. (2019) | LMC S63 (Conf.) |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | HV 12671 (Conf.) |
Right ascension (°) | 87.1810Ref | Parallax (mas) | 0.009±0.025Ref | Reddening E(B-V) (mag) | 0.1±0.02Ref, Note |
Declination (°) | -67.6029Ref | Distance (kpc) | 49.97±0.19Ref 14.04Ref, Note, 11.25Ref, Note |
||
Galactic longitude (°) | 277.6270Ref | Proper motion in α (mas/yr) | 1.50±0.03Ref | ||
Galactic latitude (°) | -30.8790Ref | Proper motion in δ (mas/yr) | 0.83±0.03Ref |
X-Ray | YesRef | IR type | SRef | Radio | - |
X-Ray type | αRef | J (mag) | 12.51Ref | Flickering | - |
GALEX FUV (mag) | - | H (mag) | 11.65Ref | Outbursts | YesRef |
GALEX NUV (mag) | - | K (mag) | 11.33Ref | Outburst type | Z And?Ref |
IUE | YesRef | WISE W1 (mag) | 11.01Ref | Jets | - |
FUSE | NoRef | WISE W2 (mag) | 11.07Ref | Resolved nebula | - |
U (mag) | - | WISE W3 (mag) | 10.54Ref | IPmax (eV) | 97.1Ref |
B (mag) | 16.71Ref | WISE W4 (mag) | 9.36Ref | [O III] lines | YesRef |
V (mag) | 15.51Ref | IRAS 12μm (Jy) | - | He II lines | YesRef |
R (mag) | 15.17Ref | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
I (mag) | 14.07Ref | IRAS 60μm (Jy) | - | O VI lines | NoRef |
BP (mag) | 15.96Ref | IRAS 100μm (Jy) | - | ||
G (mag) | 15.10Ref | AKARI S09 (Jy) | - | ||
RP (mag) | 14.14Ref | AKARI S18 (Jy) | - |
Orbital period (days) | 1050±0.5Ref | γ velocity (km/h) | 296.12±2.71Ref | Size of giant’s orbit (AU) | - |
Eccentricity | - | RV of giant (km/h) | - | Separation (AU) | - |
Inclination (°) | - | Inferior conj. of giant (JD) | - | Mass function | - |
Eclipses | YesRef | Mass ratio | - | ||
Orbital ephemeris | Min (B) = 2449885.6±7.4 + 1050±0.5 x ERef |
Spectral type | C2.1JRef | Mass (M⊙) | 2Ref | Pulsation | YesRef |
Eff. temperature (K) | 3500±250Ref | Radius (R⊙) | 190230±-Ref | Type | - |
IR type | SRef | Luminosity (L⊙) | 9120Ref, 3900Ref | Pulsation period (days) | 72±1Ref |
Metallicity [Fe/H] | - | Pulsation ephemeris | Min(I) = 2456035±1 + 72±1 x ERef |
Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
Shell-burning/Accreting-only | shell-burningRef | Radius (R⊙) | 0.4Ref | Accretion disk | - |
Eff. temperature (K) | 85000Ref, 100000Ref | Luminosity (L⊙) | 7500Ref, 1600Ref | ||
Lower limit (K) | - | ||||
Upper limit (K) | - |
The giant companion was spectroscopically classified as a carbon star. The photographic light curve revealed a 2.5 mag outburst that started in 1930, and the star remained active in the optical for at least 14 years (Iłkiewicz et al., 2015).