CONFIRMED
MILKY WAY
|
| AE Cir | IRAS - | GSC2.4.2 S7UY009737 | AAVSO 000-BCV-475 |
| SIMBAD V* AE Cir | Pan-STARRS - | SAO - | VSX 9458 |
| GAIA DR3 5799841957262188928 | SkyMapper 144451.33-692334.5 | WRAY 15-1240 | GCVS AE Cir |
| 2MASS J14445133-6923345 | HIP - | Hen 3-1025 | BD - |
| WISE J144451.31-692334.5 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | AE Cir (Susp.) |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | AE Cir (Conf.) |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 221.2138Ref | Parallax (mas) | 0.114±0.022Ref | Reddening E(B-V) (mag) | 0.23±0.0Ref, Note |
| Declination (°) | -69.3930Ref | Distance (kpc) | 9.4Ref 8.01Ref, Note, 7.77Ref, Note |
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| Galactic longitude (°) | 312.6671Ref | Proper motion in α (mas/yr) | -4.94±0.02Ref | ||
| Galactic latitude (°) | -8.6936Ref | Proper motion in δ (mas/yr) | -1.34±0.02Ref |
| X-Ray | - | IR type | SRef | Radio | - |
| X-Ray type | - | J (mag) | 10.88Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 10.05Ref | Outbursts | YesRef |
| GALEX NUV (mag) | - | K (mag) | 9.74Ref | Outburst type | Z AndRef |
| IUE | NoRef | WISE W1 (mag) | 9.46Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 9.27Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 8.22Ref | IPmax (eV) | 114Ref |
| B (mag) | 15.37Ref | WISE W4 (mag) | 7.34Ref | [O III] lines | - |
| V (mag) | 13.00Ref | IRAS 12μm (Jy) | - | He II lines | - |
| R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | - |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | YesRef |
| BP (mag) | 13.34Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 12.61Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 11.80Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | 342±15Ref | 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 | - | Mass ratio | 1.1Ref | ||
| Orbital ephemeris | Min (V) = 2447327.3±3.4 + 342±15 x ERef |
| Spectral type | K5 IIIRef | Mass (M⊙) | 1.1Ref | Pulsation | - |
| Eff. temperature (K) | - | Radius (R⊙) | 99Ref | Type | - |
| IR type | SRef | Luminosity (L⊙) | - | Pulsation period (days) | - |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | WDRef | Mass (M⊙) | 1Ref | Spin period (min) | 27.3Ref |
| Shell-burning/Accreting-only | shell-burningRef | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | 114000Ref | ||||
| Upper limit (K) | 250000Ref |
Discovered as a variable star by Swope (1931), who initially classified it as an R CrB star. Its potential symbiotic nature was suspected by Kilkenny (1989), where H I, He I, He II, and other emission lines were reported. The paper mentioned periodicities of 3900 and 100 days based on visual observations. However, Lawson & Cottrell (1990) argued that the 3900-day period does not represent the long-term variability of the system. Confirming its symbiotic nature, Mennickent et al. (2008) detected O VI 6825 lines in the spectrum and reported repeated outbursts.