POSSIBLE
MILKY WAY
|
| PPA J1807-3428 | IRAS - | GSC2.4.2 S9PF094097 | AAVSO - |
| SIMBAD [KW2003] 91 | Pan-STARRS - | SAO - | VSX - |
| GAIA DR3 4039519962898625920 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J18072317-3428508 | HIP - | Hen - | BD - |
| WISE J180723.17-342851.0 | 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 (°) | 271.8466Ref | Parallax (mas) | 0.069±0.056Ref | Reddening E(B-V) (mag) | 0.31±0.01Ref, Note |
| Declination (°) | -34.4809Ref | Distance (kpc) | 6.83Ref, Note, 7.61Ref, Note | ||
| Galactic longitude (°) | 357.5022Ref | Proper motion in α (mas/yr) | -2.93±0.06Ref | ||
| Galactic latitude (°) | -6.7767Ref | Proper motion in δ (mas/yr) | -4.41±0.04Ref |
| X-Ray | - | IR type | S?Ref | Radio | - |
| X-Ray type | - | J (mag) | 9.21Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 8.04Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 7.54Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 7.12Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 6.96Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 6.11Ref | IPmax (eV) | 35.1Ref |
| B (mag) | - | WISE W4 (mag) | 5.52Ref | [O III] lines | YesRef |
| V (mag) | 18.00Ref | 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) | 16.89Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 14.11Ref | AKARI S09 (Jy) | 0.21Ref | ||
| RP (mag) | 12.57Ref | 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 | - | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
Classified as a symbiotic star candidate in the HASH Database of PNe (Parker et al., 2016), this object exhibits a spectrum characterized by red continuum, Balmer lines, and emission lines of [O III].