POSSIBLE
MILKY WAY
|
| PM 1-286 | IRAS 19092+1326 | GSC2.4.2 N2D7029221 | AAVSO - |
| SIMBAD IRAS 19092+1326 | Pan-STARRS 124222878993294288 | SAO - | VSX - |
| GAIA DR3 4314096397510483456 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J19113584+1331113 | HIP - | Hen - | BD - |
| WISE J191135.83+133111.3 | 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 (°) | 287.8993Ref | Parallax (mas) | -0.427±0.327Ref | Reddening E(B-V) (mag) | 1.93±0.12Ref, Note |
| Declination (°) | 13.5198Ref | Distance (kpc) | 8.61Ref, Note, 4.00Ref, Note | ||
| Galactic longitude (°) | 47.2394Ref | Proper motion in α (mas/yr) | -1.07±0.27Ref | ||
| Galactic latitude (°) | 1.7526Ref | Proper motion in δ (mas/yr) | -4.22±0.25Ref |
| X-Ray | - | IR type | D'?Ref | Radio | YesRef |
| X-Ray type | - | J (mag) | 14.54Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 13.58Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 12.01Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 9.46Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 7.70Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 3.57Ref | IPmax (eV) | 99Ref |
| B (mag) | - | WISE W4 (mag) | 0.38Ref | [O III] lines | YesRef |
| V (mag) | - | IRAS 12μm (Jy) | 1.48Ref | He II lines | YesRef |
| R (mag) | - | IRAS 25μm (Jy) | 7.07Ref | [Fe VII] lines | YesRef |
| I (mag) | - | IRAS 60μm (Jy) | 7.16Ref | O VI lines | NoRef |
| BP (mag) | 18.59Ref | IRAS 100μm (Jy) | 14.80Ref | ||
| G (mag) | 18.25Ref | AKARI S09 (Jy) | 0.78Ref | ||
| RP (mag) | 16.67Ref | AKARI S18 (Jy) | 3.87Ref |
| 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 | D'?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 possible PN in the HASH Database of PNe (Parker et al., 2016), with a note about a potential symbiotic nature. While no spectrum is available in the database, a study by van de Steene et al. (1996) reported emission lines with ionization potential up to [Fe VII].