CONFIRMED
MILKY WAY
|
| K 3-12 | IRAS - | GSC2.4.2 N1QG018934 | AAVSO 000-BLH-237 |
| SIMBAD IPHAS J184446.08+060703.5 | Pan-STARRS 115342811919991678 | SAO - | VSX 238533 |
| GAIA DR3 4285602484899363456 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J18444608+0607035 | HIP - | Hen - | BD - |
| WISE J184446.08+060703.5 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | IPHASJ184446.08+060703.5 (Conf.) |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 281.1920Ref | Parallax (mas) | 0.009±0.034Ref | Reddening E(B-V) (mag) | 1.0±0.03Ref, Note |
| Declination (°) | 6.1176Ref | Distance (kpc) | 3.6Ref 10.32Ref, Note, 8.56Ref, Note |
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| Galactic longitude (°) | 37.6285Ref | Proper motion in α (mas/yr) | -1.87±0.03Ref | ||
| Galactic latitude (°) | 4.2636Ref | Proper motion in δ (mas/yr) | -3.83±0.03Ref |
| X-Ray | NoRef | IR type | SRef | Radio | - |
| X-Ray type | - | J (mag) | 11.04Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 9.88Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 9.41Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 9.00Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 8.99Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 8.46Ref | IPmax (eV) | 114Ref |
| B (mag) | - | WISE W4 (mag) | 7.88Ref | [O III] lines | NoRef |
| V (mag) | - | IRAS 12μm (Jy) | - | He II lines | YesRef |
| R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | YesRef |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | YesRef |
| BP (mag) | 16.45Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 14.72Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 13.45Ref | 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 | M2.0Ref | Mass (M⊙) | - | Pulsation | - |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | - |
| IR type | SRef | Luminosity (L⊙) | - | Pulsation period (days) | - |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | shell-burningRef | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
Listed in the catalogue of planetary nebulae, it was suspected to be a symbiotic star according to Acker & Stenholm (1990). New observations confirmed its symbiotic nature, as revealed by the emission line spectrum combined with strong 6825 and 7082 Raman-scattered lines and, albeit shallow, TiO bands, as reported in Corradi et al. (2010).