POSSIBLE
MILKY WAY
|
| V748 Cen | IRAS - | GSC2.4.2 S9H9000102 | AAVSO 000-BDK-920 |
| SIMBAD V* V748 Cen | Pan-STARRS - | SAO - | VSX 8045 |
| GAIA DR3 6204217186929931520 | SkyMapper 145936.68-332504.0 | WRAY - | GCVS V0748 Cen |
| 2MASS J14593668-3325040 | HIP - | Hen 3-1045 | BD - |
| WISE J145936.67-332504.1 | TYC 7302-2324-1 | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | V748 Cen (Susp.) |
| Gaposchkin (1957) | - | Kenyon (1986) | V748 Cen (Susp.) | Akras et al. (2019) | V748 Cen (Susp.) |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | V748 Cen (Conf.) |
| Right ascension (°) | 224.9028Ref | Parallax (mas) | 0.105±0.031Ref | Reddening E(B-V) (mag) | 0.12±0.0Ref, Note |
| Declination (°) | -33.4178Ref | Distance (kpc) | 7.01Ref, Note, 7.23Ref, Note | ||
| Galactic longitude (°) | 331.5163Ref | Proper motion in α (mas/yr) | -6.18±0.04Ref | ||
| Galactic latitude (°) | 22.2438Ref | Proper motion in δ (mas/yr) | -5.45±0.04Ref |
| X-Ray | NoRef | IR type | S?Ref | Radio | - |
| X-Ray type | - | J (mag) | 9.20Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 8.40Ref | Outbursts | YesRef |
| GALEX NUV (mag) | - | K (mag) | 8.12Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 7.96Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 7.94Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 7.58Ref | IPmax (eV) | 13.6Ref |
| B (mag) | 11.53Ref | WISE W4 (mag) | 7.17Ref | [O III] lines | NoRef |
| V (mag) | 11.27Ref | IRAS 12μm (Jy) | - | He II lines | NoRef |
| R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | NoRef |
| BP (mag) | 11.40Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 11.07Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 10.48Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | 566.5Ref | γ velocity (km/h) | - | 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 (V) = 2441917 + 566.5 x ERef |
| Spectral type | M4-5 IIIRef, M3 IIIRef | Mass (M⊙) | - | Pulsation | - |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | - |
| IR type | S?Ref | Luminosity (L⊙) | - | Pulsation period (days) | - |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | - | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
Suspected of being a symbiotic star by Kenyon (1986), the system exhibits characteristics such as an M giant continuum, UV excess, and emission lines with low ionization potential (van Genderen et al., 1974; van Genderen, 1979,Schulte-Ladbeck, 1988). Eclipses have been observed in the system (van Genderen et al., 1974; van Genderen, 1979). The symbiotic nature is further supported by the analysis presented in Akras et al. (2019).