LIKELY
MILKY WAY
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| [DWS97] Cet 7 | IRAS - | GSC2.4.2 S0NU000034 | AAVSO 000-BLM-588 |
| SIMBAD 2MASS J01093484-0800329 | Pan-STARRS 98380173951599388 | SAO - | VSX 132036 |
| GAIA DR3 2474999750706913536 | SkyMapper 010934.83-080032.9 | WRAY - | GCVS - |
| 2MASS J01093484-0800329 | HIP - | Hen - | BD - |
| WISE J010934.84-080033.1 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 17.3952Ref | Parallax (mas) | -0.018±0.033Ref | Reddening E(B-V) (mag) | 0.05±0.0Ref, Note |
| Declination (°) | -8.0092Ref | Distance (kpc) | 11.91Ref, Note, 7.78Ref, Note | ||
| Galactic longitude (°) | 136.4344Ref | Proper motion in α (mas/yr) | 0.67±0.05Ref | ||
| Galactic latitude (°) | -70.4038Ref | Proper motion in δ (mas/yr) | -0.55±0.05Ref |
| X-Ray | - | IR type | S?Ref | Radio | - |
| X-Ray type | - | J (mag) | 13.70Ref | Flickering | - |
| GALEX FUV (mag) | 18.18Ref | H (mag) | 13.38Ref | Outbursts | Yes?Ref |
| GALEX NUV (mag) | 17.66Ref | K (mag) | 12.71Ref | Outburst type | SyN?Ref |
| IUE | NoRef | WISE W1 (mag) | 12.06Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 11.48Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 9.68Ref | IPmax (eV) | 35.1Ref |
| B (mag) | 15.65Ref | WISE W4 (mag) | 5.97Ref | [O III] lines | YesRef |
| V (mag) | 15.14Ref | 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) | 15.10Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 14.80Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 14.23Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | - | 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 | - | ||
| Orbital ephemeris | - |
| Spectral type | - | 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 | shell-burning?Ref | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
The star was previously classified as a nova-like CV in Kopylov et al. (1988). However, in Honeycutt & Kafka (2010), it was suggested that it might be a symbiotic binary in a prolonged outburst. The spectrum shows He II in emission, in addition to Balmer lines and He I.