SUSPECTED
MILKY WAY
|
| PPA J1744-3252 | IRAS 17411-3250 | GSC2.4.2 S8HB178971 | AAVSO - |
| SIMBAD PN G356.5-01.8 | Pan-STARRS - | SAO - | VSX - |
| GAIA DR3 4054021657927221888 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J17442792-3252098 | HIP - | Hen - | BD - |
| WISE - | 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 (°) | 266.1163Ref | Parallax (mas) | 0.043±0.239Ref | Reddening E(B-V) (mag) | 2.11±0.14Ref, Note |
| Declination (°) | -32.8694Ref | Distance (kpc) | 7.01Ref, Note, 5.40Ref, Note | ||
| Galactic longitude (°) | 356.5150Ref | Proper motion in α (mas/yr) | -3.16±0.26Ref | ||
| Galactic latitude (°) | -1.8412Ref | Proper motion in δ (mas/yr) | -5.90±0.15Ref |
| X-Ray | - | IR type | - | Radio | YesRef |
| X-Ray type | - | J (mag) | 13.58Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 12.25Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 11.62Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | - | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | - | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | - | IPmax (eV) | 35.1Ref |
| B (mag) | - | WISE W4 (mag) | - | [O III] lines | YesRef |
| V (mag) | - | IRAS 12μm (Jy) | 3.74Ref | He II lines | NoRef |
| R (mag) | - | IRAS 25μm (Jy) | 1.92Ref | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | 6.38Ref | O VI lines | NoRef |
| BP (mag) | 20.61Ref | IRAS 100μm (Jy) | 345.00Ref | ||
| G (mag) | 18.64Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 16.93Ref | AKARI S18 (Jy) | 0.89Ref |
| 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 | - | 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) | - |
Classified as a true PN in the HASH Database of PNe (Parker et al., 2016), the central star of this PN might be a symbiotic star or a Mira-type variable, according to notes in the database. The spectra show Balmer lines in emission, [O III] lines, and faint He I.